The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its shape is generally round, exhibiting minimal elongation. There's no discernible evidence of spiral arms or a prominent disk structure. The light distribution suggests a lack of significant dust lanes or patchy star formation. The central region displays a slightly yellowish hue, likely indicating a population of older stars, with the outer edges of the galaxy fading smoothly into the background sky. There does not appear to be any evidence of ongoing major merger activity or significant tidal distortions in the galaxy's shape.
