The galaxy presents as a single, relatively concentrated object with a roughly elliptical morphology. The central region exhibits a brighter, more intensely luminous core, suggesting a higher stellar density in that area. The overall color profile indicates a bias towards redder wavelengths, which may be indicative of an older stellar population, reduced star formation activity, and/or a higher dust content within the galaxy. There is a faint extension on one side of the galaxy that may indicate interaction with a smaller galaxy, or otherwise, a possible tidal feature of the system. There are no clearly defined spiral arms, but the galaxy is relatively round in shape. The galaxy appears quite compact, and is relatively smooth in appearance. 
