The galaxy presents as a centrally concentrated object, roughly elliptical in shape. The core region exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy appears to fade in intensity, transitioning to a more diffuse, greenish-yellow color. There is little evidence of distinct spiral arms or significant dust lanes. The overall smoothness of the light distribution indicates a relatively evolved system, consistent with a galaxy dominated by older stars and a less active star formation rate. Slight disturbances on the outer edges indicate the possibility of minor gravitational interaction with another object.
