The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated, bright core that gradually diffuses outwards. The overall color profile suggests an older stellar population, with a greater concentration of light towards the redder end of the spectrum. There is minimal evidence of significant dust lanes or prominent spiral arm structures, which further supports its classification as an elliptical galaxy. The galaxy appears relatively isolated, showing no obvious signs of recent or ongoing major merger events or tidal interactions. There may be minor distortions, but they are not prominent. The shape is close to round but not perfectly round, and not cigar shaped. Overall, the image portrays a well-formed, mature galaxy with a high likelihood of low star formation activity.
