The galaxy presents an overall smooth morphology, exhibiting a relatively featureless light distribution with an apparent lack of distinct spiral arms or a prominent bar structure. The central region displays a concentrated, bright core, which is suggestive of a significant stellar population and potentially an active galactic nucleus.

The galaxy exhibits a slightly elliptical shape. The color profile suggests a dominance of older stellar populations, particularly in the central bulge, indicated by the yellow-orange hue. Fainter bluish regions suggest the presence of some younger, hotter stars and potential ongoing, though limited, star formation. There is no evidence of a major ongoing merger. The morphology is largely undisturbed, though there is a small region that could be a minor disturbance. The galaxy does not have a clear disk.
