The galaxy presents as a primarily smooth and rounded structure, appearing elliptical in shape with a bright central bulge dominating the luminosity profile. A faint, diffuse halo surrounds the central region, hinting at a larger galactic extent. There is evidence of a minor disturbance or interaction on the left side of the galaxy, appearing as an irregularity of color or slight tidal feature. The blueish hue suggests a moderate amount of star formation is present within the system, though overall, the galaxy appears to be in a relatively quiescent state. The stellar population is a mix of older and younger stars, as indicated by the presence of both redder and bluer colors. Based on this observation, the galaxy is most likely a lenticular or early-type spiral galaxy undergoing minor interactions. 
