The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a distinct yellowish-red hue, indicating a population of older stars and a lack of significant ongoing star formation. The galaxy is generally round in shape, with no obvious spiral arm structures or other prominent features typically associated with disk galaxies. There is little evidence of recent or ongoing mergers or tidal disturbances. The galaxy's overall morphology suggests a classification as an early-type galaxy with a quiescent stellar population.
