The galaxy appears as a relatively smooth, elliptical-shaped structure, with a discernible central bulge. There is a slight elongation, suggesting it is not perfectly spherical but somewhat cigar shaped. The overall color gradient indicates a population of older stars, leaning towards redder hues. There is no obvious evidence of ongoing, intense star formation regions or dust lanes. Some minor disturbances or tidal features may be present, but the galaxy seems mostly undisturbed in terms of merging activity. The morphology gives it the appearance of an early-type galaxy, most likely an elliptical or lenticular.