The galaxy presents a generally smooth morphology, appearing largely featureless in the available image. It exhibits a centrally concentrated luminosity profile, with light intensity gradually decreasing towards the outer regions. The overall shape appears roughly circular, displaying only a minor deviation from perfect sphericity. There is a suggestion of a slightly disturbed morphology, with possible minor asymmetries, that may be indicative of past or ongoing interactions. The galaxy displays a color gradient, with the central region appearing yellowish-white and the outer regions transitioning to bluer hues. This suggests that the central region is dominated by an older stellar population, whereas the outer regions may have younger, bluer stars or be undergoing star formation. The moderate luminosity of the galaxy points towards a relatively low rate of star formation. Despite its smooth appearance, a slight disturbance is present. Overall, the galaxy exhibits characteristics consistent with a galaxy in the early stages of morphological transformation or having experienced minor gravitational interactions.
