The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The morphology is predominantly smooth, lacking any prominent spiral arms or distinct disk-like features. The color profile indicates a population of older stars, with a yellowish-red hue dominating the core region. There may be some evidence of ongoing, but low levels, of star formation in the outer regions. The overall roundness suggests a classification closer to E0-E3 on the Hubble sequence. There are no apparent signs of major mergers or tidal disturbances, although some subtle irregularities hint at possible minor interactions in the past. The galaxy's moderate redshift indicates that it is a distant object.
