The galaxy presents a primarily smooth morphology, with a slight hint of disc-like structure. The overall shape is largely round, with a subtle elongation. The central region exhibits a bright, concentrated luminosity, suggestive of a significant bulge. The color profile indicates a higher concentration of older stars. The galaxy does not appear to be undergoing any major merging events, though there may be some minor tidal disturbances. Overall, the galaxy appears as a relatively massive galaxy with a low specific star formation rate.
