The galaxy presents a largely featureless morphology, appearing smooth and elliptical in shape. The light distribution is concentrated towards the center, with a bright, nearly circular core that diminishes in intensity toward the outer edges. The color appears reddish-yellow, suggestive of an older stellar population. There are no obvious spiral arms or dust lanes visible, and it shows no signs of a recent or ongoing major merger. The overall appearance indicates that this is a well-formed galaxy in a relatively stable state. Slight irregularities in color distribution suggest some degree of substructure or ongoing minor interactions, but these are subtle. The galaxy appears to be relatively isolated.
