The galaxy presents as a single, relatively symmetrical object. Its overall shape appears to be elliptical, exhibiting a high degree of roundness with only a slight deviation toward a cigar-like shape. The galaxy's light profile is smooth and concentrated toward the center. There's no clear evidence of spiral arm structures or prominent dust lanes. The color suggests a population of older stars, given its reddish hue. There is no apparent tidal disruption, or nearby companions that would lead to the presence of a major or minor merger event, or disturbed features.
