This galaxy exhibits an elliptical morphology, appearing relatively smooth and lacking prominent spiral arm structures. The galaxy displays a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. It is not perfectly circular, but appears slightly elongated, showing a small degree of ellipticity. The color profile suggests a predominantly older stellar population, with a light blue hue in the central region, likely attributed to a recent epoch of star formation or the presence of a blue stellar population. There is a subtle suggestion of minor disturbances in the outer regions, potentially indicative of a past or ongoing interaction, but it does not seem to be undergoing a major merger. The object's regular shape points away from any major tidal distortion.
