This galaxy appears to be an elliptical galaxy, potentially of type E4-E6, viewed nearly edge-on. The central bulge exhibits a concentrated, yellowish hue, suggestive of an older stellar population dominated by evolved stars. Fainter, bluer light extends outwards from the bulge in a flattened, diffuse structure, indicating the presence of a disk component. The smoothness of the overall light distribution suggests that this galaxy is likely not undergoing any major merging events, although there may be some minor asymmetry in the outer regions which could suggest some tidal interactions or minor disturbances.
