The galaxy appears as a somewhat centrally concentrated object, exhibiting a smooth morphology with little indication of spiral arm structures or prominent features. Its overall shape can be described as slightly elongated, perhaps best characterized as an intermediate form between round and cigar-shaped. There is a hint of a disk or a subtle feature. The galaxy is mostly composed of older stellar populations, as inferred from the reddish color, suggesting relatively low ongoing star formation activity. The object does not appear to be undergoing any major merging events, with only minor disturbances, if any, visible in its structure. The estimated size suggests a relatively compact galaxy.
