The galaxy presents a predominantly smooth morphology, exhibiting a concentrated central bulge that diminishes gradually into a less defined outer region. The color profile indicates an evolved stellar population, displaying a yellowish-orange hue centrally, suggestive of older stars. There is no discernible spiral structure or prominent dust lanes. The galaxy appears elliptical in shape, with a high degree of roundness. There is no evidence of ongoing major mergers or significant tidal disturbances. Star formation activity appears low.
