The galaxy appears as a central, concentrated luminosity with a largely smooth morphology. Its overall shape is elliptical, appearing fairly round with only slight deviations from circular symmetry. There is a subtle color gradient, with a core that appears more yellow-orange, suggesting older stellar populations, grading to a slightly bluer hue in the outer regions. There are no obvious spiral arm structures or prominent dust lanes visible. The galaxy exhibits no strong evidence of ongoing major mergers or significant tidal disturbances.
