The galaxy presents as a generally smooth, centrally concentrated object. It appears elliptical in shape, with the major axis slightly elongated relative to the minor axis, giving it a somewhat cigar-shaped appearance. The light distribution is characterized by a bright central core, diminishing in intensity outward, with no obvious spiral arm structure or prominent dust lanes visible. The color profile suggests a dominant population of older stars, with a yellowish hue indicative of lower star formation rates, consistent with a more evolved stellar population. There are no apparent signs of tidal disturbances, close companion galaxies, or ongoing major merger events. Minor irregularities cannot be ruled out due to image resolution.
