The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with a central concentration. The luminosity profile suggests a relatively homogeneous stellar population. The color gradient across the galaxy is subtle, with a tendency towards redder hues in the core regions transitioning towards slightly bluer tones in the outer edges. There is no obvious evidence of spiral arms or prominent dust lanes. Based on the visual characteristics, this galaxy appears to be a well-formed, relatively quiescent system.
