The galaxy presents an elliptical morphology, appearing relatively smooth with a concentrated central bulge. There is a slight elongation observed, however the overall shape is close to round. Evidence of a disk structure is minimal to non-existent. No distinct spiral arms or prominent dust lanes are visible. The color gradient suggests a predominantly older stellar population, as indicated by the reddish hue, especially in the core region. Star formation appears to be suppressed or at a very low rate within the galaxy. There might be a faint, diffuse halo surrounding the core, but it's difficult to ascertain the exact extent due to background noise. There are no readily apparent signs of any recent or ongoing major merger activity, though some minor disturbances cannot be entirely ruled out. Overall, the galaxy presents itself as a mature, relatively quiescent system.
