The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a centrally concentrated brightness profile. There are no discernible spiral arms or significant dust lanes visible in the image. The galaxy displays a yellow-orange hue, suggesting a stellar population dominated by older, redder stars, indicative of lower star formation activity. It is mostly round in shape. There is no obvious evidence of major mergers or significant tidal disturbances in the image.
