This galaxy exhibits a generally smooth morphology, suggestive of an elliptical or lenticular type. The central region displays a concentrated, bright yellowish-orange hue, potentially indicative of an older stellar population dominating the core. The galaxy appears somewhat elongated, with an axis ratio that deviates from perfectly circular. There is a subtle color gradient noticeable from the core outwards, transitioning towards a dimmer, bluish-greenish tint in the outer regions. This might suggest the presence of some younger stars or ongoing star formation, albeit at a low rate in the outskirts. No prominent spiral arms or distinct dust lanes are visible. There is no obvious evidence of significant tidal disturbances or interactions with other galaxies.
