The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth light distribution, with a bright core that gradually fades into the outer regions. The color profile suggests a relatively older stellar population. The galaxy is elongated, with a major axis roughly twice the length of its minor axis. There is no discernible spiral structure or prominent dust lanes. Faint, diffuse light extends outwards from the main body of the galaxy, indicating a possible halo or extended stellar envelope. There is no evidence of any ongoing major merger activity or significant tidal disturbances in the image.
