This galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is somewhat round, although there is a slight elongation. The galaxy exhibits a prominent central bulge, characterized by a bright, yellowish hue, suggesting a population of older stars. There is a hint of a fainter, more diffuse disk component extending outwards from the bulge, primarily visible as a faint, blueish extension on one side. While the galaxy is generally smooth in appearance, subtle irregularities in the light distribution suggest the possibility of minor disturbances, perhaps due to past interactions or mergers. Overall, the system is reasonably massive and appears to have a low star formation rate.
