The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, with the light intensity decreasing gradually towards the outer regions. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue, particularly in the core. There is minimal evidence of spiral arm structure or significant dust lanes. A faint blueish tint is present in the outskirts, possibly indicating some recent star formation, though limited. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Its shape is more rounded than elongated. The size is estimated to be around 7 kpc.
