The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The major axis is significantly longer than the minor axis, giving the galaxy a distinctly elongated, cigar-like appearance. The central region displays a bright, concentrated core, suggesting a possible bulge. The light from the core gradually fades outwards towards the edges of the galaxy, with no apparent spiral arm structures. The overall color appears yellowish-white, suggesting an older stellar population with a relatively low rate of ongoing star formation. There is a subtle color gradient, with the core appearing slightly more yellow. The galaxy appears relatively undisturbed with no signs of major mergers or tidal interactions. The edges of the galaxy are rather diffuse, suggesting a possible halo component, but it appears to be compact.
