The galaxy presents a largely smooth morphology, with minimal discernible features suggesting a disk or spiral structure. Its shape appears somewhere between round and elongated, without a significant cigar-like aspect. The light distribution is centrally concentrated, with a bright core that gradually fades towards the outer regions. Color gradients are subtle, showing a general bluer hue towards the center that transitions to redder tones at the periphery. There is no obvious evidence of major mergers or significant tidal disturbances in its immediate vicinity. The overall appearance suggests a relatively evolved system, with a considerable amount of its stellar population being older. Star formation rate appears to be present, although at intermediate levels. Estimated mass of the galaxy falls within a intermediate range.
