The galaxy presents as a generally smooth, elliptical structure, elongated in a roughly northwest-southeast direction. The core region appears significantly brighter and more concentrated than the outer regions. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central bulge. Fainter, greenish tinges are observed towards the outer edges, possibly indicating the presence of some younger stars or ionized gas, though this is not strongly evident. No distinct spiral arm structures or prominent dust lanes are discernible within the galaxy's image. The overall morphology points towards a relatively evolved system, likely a galaxy that has largely completed its major star-forming epoch. The shape is somewhat cigar-like rather than perfectly round, and its mass and star formation rate are moderate.
