The galaxy presents as a concentrated, centrally brightened system. The light distribution appears relatively smooth with a high degree of circular symmetry. There is no visible evidence of spiral arm structure or a prominent disk. The galaxy exhibits a color gradient, appearing more yellow-gold towards the center and becoming slightly redder in the outer regions. This suggests a concentration of older stellar populations in the core. No significant signs of tidal disturbances, major mergers, or ongoing star formation are apparent from this image. The galaxy is compact and well-defined, indicative of a relatively quiescent system.
