The galaxy presents as a relatively smooth, featureless object. Its morphology appears elliptical, with a slightly elongated shape. The color profile indicates a redder hue, suggesting a population of older stars and relatively low ongoing star formation. There is no evidence of spiral arms or a prominent central bulge. The light distribution appears concentrated toward the center, gradually fading into the background. No signs of significant tidal interactions or ongoing mergers are readily apparent, though minor disturbances cannot be ruled out at this resolution. The overall appearance suggests an evolved galaxy with a dominant population of older stars, likely classified as an elliptical galaxy.