The galaxy appears as a slightly elongated, diffuse object with a relatively smooth overall structure. Its color profile suggests a dominant older stellar population. However, there is some subtle color variation, possibly indicative of ongoing, low-level star formation. The galaxy does not display strong spiral arm features or a pronounced central bulge, lending it a more amorphous appearance. There are no obvious signs of a major ongoing merger, although some slight asymmetry may suggest past interactions or minor disturbances. The lack of prominent dust lanes is also noticeable. Overall, the galaxy presents as a moderately massive system with intermediate characteristics, potentially representing a transitional stage in galaxy evolution.
