The galaxy presents a generally smooth, elliptical morphology with a slight elongation. The central bulge is prominent and exhibits a concentrated luminosity. The galaxy displays a color gradient, with the core appearing yellower, suggesting a population of older stars. The outer regions are somewhat bluer in comparison, potentially indicating areas of more recent star formation. There is no clear evidence of a prominent disk structure or spiral arms. Minimal visible dust lanes or morphological disturbances suggest a relatively settled state, with no apparent major ongoing mergers. There may be a slight hint of minor tidal features. Overall, the galaxy appears to be an intermediate-mass system.
