The galaxy presents as a roughly elliptical morphology with a prominent, centrally concentrated bulge. A faint, extended disk is suspected, exhibiting low surface brightness. The central region displays a bright, concentrated core, potentially indicative of an active galactic nucleus or a dense stellar population. The color profile suggests a complex stellar population. The central bulge exhibits a bluer hue, implying the presence of younger, hotter stars, or ongoing star formation. This is surrounded by what looks to be a redder rim around the ellipse. Faint asymmetries or distortions are observed in the outer regions, possibly suggestive of past minor merger events or tidal interactions. There appears to be a slight extension on one side, hinting at potential disturbances.
