The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a concentrated, bright central region, possibly indicating a substantial galactic nucleus. The overall shape is largely spheroid, with minimal discernible disk features or spiral arms. There are some slight irregular features within the galaxy's outer halo. The galaxy's color profile suggests a dominant population of older stars and a low rate of ongoing star formation, with a redder hue dominating the visual representation. There is little evidence of a major ongoing merger event, although some minor disturbances cannot be ruled out.
