The object appears as a single, moderately bright galaxy. It exhibits a generally smooth morphology, with no readily discernible spiral arms or bar structure. The galaxy presents a centrally concentrated luminosity profile, gradually diminishing outward. The color index suggests the galaxy is relatively red, potentially indicating an older stellar population and/or significant dust content. The galaxy has a relatively circular appearance. There is no evidence of a major ongoing merger or strong tidal interaction from what can be seen in the image.
