The galaxy presents a predominantly smooth morphology, with a centrally concentrated luminosity profile. There is an apparent lack of distinct spiral arm structures. The galaxy appears to be neither perfectly elliptical nor a well-defined spiral, displaying characteristics of an intermediate type, possibly a lenticular galaxy. The central region exhibits a yellowish hue, potentially indicating an older stellar population, while the outer regions possess a slightly bluer color, possibly representing regions of ongoing, albeit subdued, star formation. There appears to be a minor asymmetry or disturbance in the morphology, possibly indicating a past or ongoing minor merger event. Overall, the galaxy appears to be a relatively massive system, with moderate levels of star formation activity.
