The galaxy presents a generally smooth, elliptical morphology. Its color profile indicates a population of older stars, exhibiting a reddish-yellow hue concentrated towards the center of the galaxy, which is characteristic of galaxies with minimal active star formation. A slight extension along a particular axis indicates a subtle deviation from perfect circularity, though it remains generally rounded. There is no discernible evidence of spiral arms, bars, or significant dust lanes. The overall structure appears undisturbed, suggesting a lack of recent major mergers or tidal interactions with neighboring galaxies.
