The galaxy appears to be a relatively smooth and rounded elliptical galaxy with a bright central bulge. There is little evidence of spiral arm structure or significant dust lanes. The color gradient suggests a slightly bluer central region, which could indicate the presence of younger stars or ongoing star formation, though at a low rate. The outer regions are redder, likely dominated by older stellar populations. There is no obvious sign of a major merger or significant tidal disturbances. The galaxy presents a generally undisturbed morphology.
