The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a moderate degree of roundness, lacking a distinct disk structure. There are no prominent spiral arms visible. The color profile suggests a dominant population of older stars, with the galaxy exhibiting a slightly redder hue in the visible spectrum. There is a lack of significant dust lanes or patchy star formation regions. There is an object close in proximity, which may indicate an ongoing merger or tidal interaction. The shape is not severely distorted, however, suggesting if a merger is occurring it is in its earlier stages of development. Overall the galaxy appears to be a relatively passive system with a low star formation rate.
