The galaxy presents a primarily smooth and rounded morphology. There is a concentrated central bulge region that exhibits a yellowish hue, potentially indicating an older stellar population within. Fainter, diffuse light extends outwards from the central bulge. There is little evidence of spiral arms, distinct features, or significant dust lanes that are discernible at this resolution. The galaxy's overall appearance suggests a relatively evolved system. The color profile indicates redder overall light, with a slight green hue on its edges, which may imply ongoing, albeit low-level, star formation activity.
