The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge which is bright and yellowish in color, suggesting a population of older stars. The outer regions are less defined with a gradual decline in luminosity and a subtle color shift towards redder hues. There is no apparent spiral structure or significant dust lanes visible. The galaxy presents as a single, cohesive unit, lacking any signs of major mergers or tidal disruptions. There is very slight asymmetry in the shape, perhaps hinting at minor interactions or internal dynamics. Overall, it is a typical elliptical galaxy with a smooth, featureless morphology.
