The galaxy presents an overall elliptical morphology, appearing relatively smooth with a concentrated central bulge exhibiting a yellowish-white hue. The bulge appears moderately round, transitioning gradually into a less-defined disk-like structure. This structure shows faint extensions or arms, possibly indicative of ongoing star formation, as suggested by the presence of bluish-green regions, possibly representing younger, hotter stars within these areas.

There is slight asymmetry in the galaxy's overall structure; on one side, there is a more extended and diffuse area, while the opposite side shows a more compact and defined edge. There is no strong evidence of ongoing major merging activity.
