The galaxy presents as an elliptical morphology with a relatively smooth light distribution. The core region is concentrated and bright, exhibiting a yellowish-white hue. This central region gradually diffuses outwards into a fainter, more extended halo. There is a subtle color gradient observed, with the core appearing slightly more yellow, potentially indicating an older stellar population compared to the outer regions. There is no apparent dust lane or spiral arm structure visible. Overall, the galaxy appears undisturbed, with no signs of recent merger activity or tidal features. The shape is close to circular.
