The galaxy presents a somewhat elliptical morphology, appearing more elongated than circular. It exhibits a generally smooth texture, suggestive of an evolved stellar population. A concentration of luminosity is evident in the central region, possibly indicating a galactic bulge. The color profile shows a predominantly red-yellow hue, hinting at a population of older, cooler stars. Some bluer colors are visible in the disk but less prominent overall, indicating recent star formation is likely occurring, albeit at a moderate rate. There are indications of minor disturbances or asymmetrical features, perhaps due to a past or ongoing interaction with another galaxy. This does not look like a strong interaction or merger, but the disturbance is there nonetheless.
