The galaxy presents a generally smooth and elliptical morphology. The central bulge exhibits a concentrated, bright yellowish hue, indicative of an older stellar population. The galaxy appears to have a fairly symmetrical distribution of light, with a slight elongation. There are no prominent spiral arm features visible; instead, there is a relatively smooth gradient in color and luminosity extending outwards from the core to the more diffuse outer regions. A slight asymmetry is present in the outer halo, but overall, the galaxy does not appear significantly perturbed. There are no prominent tidal tails or signs of recent major merger activity. The faint color suggests it is a relatively massive galaxy with a low star formation rate.
