The object presents as a single, relatively smooth, luminous entity. It is characterized by a centrally concentrated morphology with a gradual decrease in surface brightness towards the outer regions. The galaxy exhibits a roughly elliptical shape with moderate ellipticity, appearing mostly round. The color profile suggests a population of older stars, as indicated by the reddish-yellow hue dominating the central region. The outer halo appears more blue, suggesting younger and fewer star populations. There is no discernible spiral arm structure or dust lane visible. The overall appearance suggests an early-type galaxy, potentially an elliptical or lenticular galaxy, which would indicate an older stellar population with a relatively low rate of ongoing star formation. There is no obvious tidal features or signs of recent major merger activity. There seems to be a mild disturbance with no clear indications of merging, likely indicating a relatively isolated system or past merging event. 
