The galaxy presents a relatively smooth, elliptical morphology. It exhibits a central concentration of light that fades gradually towards the outer edges. The core appears slightly yellowish, suggestive of an older stellar population. The overall color profile suggests a lack of significant ongoing star formation. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy's shape deviates slightly from perfect circularity, indicating a possible minor interaction or internal dynamical process. There is a subtle asymmetry in the light distribution, but overall it is fairly regular in form. No signs of recent major merger events are present, but some low-level tidal features may be present upon further analysis.
