The galaxy presents an elliptical morphology, with a centrally concentrated luminosity profile. The core region exhibits a bright, smooth appearance, indicative of an older stellar population. There is a noticeable color gradient outward from the core, suggesting a gradual change in stellar populations or metallicity. Faint, diffuse extensions are visible, potentially indicating a stellar halo or tidal features. A slight distortion or asymmetry in the overall shape may hint at past or ongoing minor interactions, but there is no clear evidence of major merging events. Low levels of ongoing star formation is expected within the galaxy.
