The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, largely featureless morphology. It demonstrates a centrally concentrated luminosity profile, with a bright, unresolved core, and a gradual decrease in surface brightness towards the outer regions. The shape is generally round, with only a slight deviation towards a more elongated form. There is no clear evidence of spiral arms or a prominent disk structure. The color indices suggest a population of older stars, contributing to the yellow-reddish hue. There is no indication of active star formation regions, or any strong dust lanes. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or ongoing merger events.
