The galaxy appears as a concentrated, centrally-bright object with a relatively smooth overall profile. It exhibits a roughly elliptical morphology, appearing largely rounded with only a slight deviation from a perfectly circular shape. The central region is dominated by a bright yellowish-white light, suggesting a significant population of older stars. The light gradually diffuses outward from the core, transitioning to a reddish hue in the outer regions. The lack of prominent spiral arms or distinct features indicates that the galaxy is likely an elliptical or lenticular type. There are only minor signs of disturbance and the galaxy appears to be isolated, without any obvious interacting companions or merger activity.
