The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright core region that diminishes in intensity outwards. There is a slight elongation, it appears mostly round. There seems to be a lack of distinct spiral arms or significant dust lanes. The color profile suggests a population of older stars, with a reddish-yellow hue dominating the galaxy's overall appearance. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances, though some minor irregularities could be present. There is an absence of large, bright star-forming regions.
