The galaxy presents a largely smooth, elliptical morphology. It exhibits a radial brightness gradient, with a concentrated central bulge that diffuses outwards into a less defined halo. The color profile suggests a population of older stars, as indicated by the redder hue. There is no prominent disk structure or spiral arms visible. Indications suggest minimal ongoing star formation. The galaxy's symmetrical appearance does not indicate any recent major mergers or significant tidal disturbances. The shape appears more round than elongated. Overall, this galaxy appears to be a relatively quiescent, evolved system.
