The galaxy presents a primarily smooth morphology, with a dominant central bulge exhibiting a yellow-orange hue, suggestive of an older stellar population. A faint, diffuse disk may be present, but it is difficult to discern distinct spiral arms. The overall shape appears somewhat elliptical, though not perfectly rounded, possibly indicating an intermediate stage between elliptical and spiral classification. There is a potential indication of minor disturbances in the galaxy's structure, which may suggest tidal interactions or a past merger event. Overall, the appearance suggests a large and relatively quiescent galaxy, likely with minimal current star formation activity.
