The galaxy presents as a fairly smooth, centrally concentrated object. It displays a slightly elliptical morphology, appearing more in between round and elongated. There is no obvious presence of a disk structure or spiral arms. The galaxy core is a brighter, concentrated luminosity with a pale blue hue. Surrounding the core, the light profile fades gradually outward. Faint traces of what may be a minor tidal disturbance are visible in the upper portion of the galaxy, though overall the image does not indicate a major merger event. The galaxy exhibits a red hue, indicating a possible population of older stars. Star formation appears to be present within the central region. The overall impression is that of a quiescent galaxy with a moderate stellar mass and a low specific star formation rate.
