The galaxy presents as a smooth, centrally concentrated object. Its morphology appears elliptical, displaying a notable lack of spiral arm structures or significant dust lanes. The light profile gradually decreases from the bright central region towards the outer edges, suggesting a relatively old stellar population. The color gradient is subtle; the core exhibits a yellowish hue, transitioning to a slightly bluer tint in the outer regions, potentially indicating some ongoing, albeit modest, star formation activity. There is no obvious sign of tidal disturbances or interactions with neighboring galaxies.
