The galaxy presents a generally smooth, elliptical morphology with a noticeable central bulge. The light distribution appears concentrated towards the core, which exhibits a yellowish hue, suggesting an older stellar population. The overall shape is somewhat elongated, exhibiting a moderate ellipticity that deviates from a perfectly circular form. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions with nearby objects. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo. The color gradient suggests a slight reddening towards the center, possibly due to increased metallicity or dust absorption.
