The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a concentrated central bulge with a gradually diminishing brightness gradient towards the outer edges. The galaxy has a mildly elliptical shape, showing no distinct spiral arms or significant dust lanes within the image resolution. The color profile suggests a population of older stars, as evidenced by the redder hue, particularly towards the central region. There's little indication of ongoing major star formation. No signs of tidal disturbances, mergers, or significant interactions with neighboring galaxies are apparent in this observation. Overall, the galaxy presents a picture of a relaxed, evolved system.
