The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, suggesting a lack of prominent spiral arms or significant dust lanes. The color gradient indicates a population of older stars, likely with a suppressed star formation rate. There are hints of a faint, extended halo surrounding the main body of the galaxy, although the image resolution limits detailed analysis of its structure. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy in a relatively quiescent state.
