The galaxy presents as a relatively smooth, elliptical object, suggesting an older stellar population. The light distribution appears centrally concentrated with a gradual falloff in intensity towards the outer regions. The axial ratio indicates a slightly elongated, but mostly rounded shape. There is no visual evidence of spiral arms or significant dust lanes, contributing to its overall smooth appearance. No obvious signs of recent or ongoing major merger events are apparent, and it appears relatively undisturbed. The galaxy exhibits a moderate redshift, which would indicate that it is a significant distance from our own. Overall, the galaxy appears to be an evolved, early-type galaxy with relatively low levels of ongoing star formation.
