The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, appearing brightest at its core and gradually fading towards the outer edges. The shape is elongated, leaning more towards an in-between elliptical shape, rather than perfectly round or a cigar-like shape. There is no clear evidence of spiral arm structures or significant dust lanes. The galaxy appears isolated, showing no obvious signs of recent or ongoing major mergers or significant tidal disturbances, but a minor disturbance can't be ruled out. The galaxy's color appears to be on the redder side, suggesting an older stellar population and a relatively low current star formation rate. Overall, this galaxy likely represents an evolved system primarily composed of older stars.
