The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, exhibiting a central bulge with a high degree of sphericity. The galaxy lacks any readily discernible spiral arm structure or prominent dust lanes. There are no obvious signs of ongoing major mergers or tidal interactions. The color profile indicates a relatively red population, with a slightly more concentrated yellowish hue at the galactic center. The overall appearance suggests an evolved system, likely with a dominant population of older stars and low levels of current star formation activity.
