The galaxy presents a roughly elliptical morphology, with a smooth, concentrated central bulge. The color profile suggests an older stellar population dominates the bulge, appearing reddish. Extending from the central region, there's a notable asymmetrical feature exhibiting a bluer hue. This could indicate a region of more active star formation, possibly triggered by an interaction or internal process. The overall form is not a perfectly smooth ellipse, suggesting a mild disturbance or interaction history. There is no strong evidence of a spiral arm structure, although some faint, diffuse extensions are visible. These features could suggest a recent minor merger event or tidal disruption. The galaxy appears to be relatively isolated, lacking any immediately apparent companion galaxies that may be influencing its structure.
