The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or S0 type based on its morphology. The central bulge is quite prominent and exhibits a bright, almost stellar-like core. The light distribution appears to fall off smoothly from the center outwards, with no distinct spiral arms or significant dust lanes visible. There may be a faint, diffuse halo surrounding the brighter central region, which gives off a faint greenish color. The galaxy’s overall color is somewhat redder, suggesting a population of older stars. There does not seem to be evidence of any major mergers or significant tidal disturbances in its immediate vicinity. It exhibits a notable elongated shape.
