The galaxy appears to be a single, relatively smooth object with a slightly elliptical morphology. It presents a central bulge that is bright and concentrated. The galaxy's light profile suggests a relatively high Sersic index, indicating a centrally concentrated light distribution. There is a slight elongation in the major axis.

A faint, diffuse halo surrounds the central region, extending further along the apparent major axis. The galaxy exhibits a color gradient, appearing bluer in the outer regions and redder towards the core. This may indicate a higher proportion of younger, hotter stars in the outer regions and older, cooler stars in the center.

There appears to be minor disturbance along the galaxy, possibly indicating an ongoing interaction or merger event. The color distribution and smooth appearance of the object suggest it may be an elliptical galaxy. Its estimated size is approximately 6 kpc in radius.
