The galaxy presents a generally smooth appearance. The primary component is a bright, somewhat rounded central bulge or core. There is evidence of a fainter, more diffuse structure extending from this core, possibly indicative of a disk or tidal features. The galaxy exhibits a slight elongation, deviating from a perfectly circular form. There appears to be some level of disturbance within the galaxy, perhaps due to minor gravitational interactions or internal processes. The overall color suggests a population of older stars, as the galaxy appears more reddish in color. Further analysis with higher-resolution imaging and spectroscopic data is needed to confirm the morphology and nature of the apparent disturbances.
