The galaxy presents a largely smooth and centrally concentrated morphology. The central region exhibits a high degree of luminosity, suggesting a significant concentration of stars. The overall shape appears to be somewhat elliptical, with the light gradually diminishing from the center towards the outer edges. There is little to no visible substructure, such as spiral arms or prominent dust lanes, implying a relatively featureless disk, if present at all. The color profile seems to transition from a brighter, slightly yellow-white core to a fainter bluish hue in the outer regions, potentially indicating differing stellar populations, with older, redder stars dominating the core, and younger, bluer stars possibly more prevalent in the outer regions. There may be evidence of a minor disturbance or interaction in its recent history, although the general structure remains largely undisturbed. Based on the light profile, the galaxy is relatively compact and massive.
