The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated central bulge which appears elongated. The light distribution is diffuse, showing a gradual decline in intensity from the center outwards with no distinct spiral arm structures visible. The color gradient suggests an aging stellar population, dominated by redder hues, particularly concentrated within the central region. There appears to be evidence of a possible minor gravitational disturbance, the galaxy seems slightly disturbed from a perfectly elliptical shape. Overall, the galaxy appears to be an intermediate to massive elliptical galaxy.
