The galaxy appears to be a relatively smooth, elliptical galaxy with a moderate redshift. Its light profile is centrally concentrated, exhibiting a bright, reddish core that gradually fades into a diffuse, greenish-yellow halo. The galaxy displays a somewhat elongated shape, suggesting it may be an E4-E6 type elliptical. There is no discernible evidence of spiral arms or significant dust lanes, and the overall morphology suggests a system dominated by an older stellar population. The lack of distinct features indicates that the galaxy is likely in a relatively quiescent state, with little ongoing star formation. There are some suggestions of minor disturbances within the galaxy, such as slight asymmetry of the halo.
