The galaxy appears to be an early-type galaxy, likely elliptical or lenticular, given its generally smooth and centrally concentrated light profile. The light is concentrated in the center of the galaxy. There is no obvious spiral arm structure, and the galaxy is generally round in appearance. A slight elongation is visible, but not enough to classify it as a highly distorted or cigar-shaped morphology. The color suggests a population of older stars, with a redder hue throughout the main body. There may be some minor disturbances, like a possible tidal tail feature on the right side of the galaxy. The tidal tail is indicated by a patch of light separate from the center of the galaxy. These disturbances could be due to a past minor merger event, or tidal interactions with smaller satellite galaxies, although no obvious merging activity is immediately apparent. Overall, it appears as a relatively massive galaxy, typical of early-type galaxies found in groups or clusters.
