The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that emits a significant amount of light, suggesting a high density of stars in that region. The color of the bulge appears more yellow/orange, which could be indicative of an older stellar population. Moving outward from the center, the light gradually fades, and the overall color appears to shift slightly towards redder wavelengths. This suggests the outer regions may contain a lower density of stars, or possibly dust obscuring some of the light. There is a lack of clearly defined spiral arms or prominent dust lanes. The overall form appears fairly regular, without any major signs of tidal disruption or ongoing major mergers, though minor disturbances can't be ruled out.
