The galaxy presents a generally elliptical morphology, though some irregularities in its outer regions hint at a more complex structure. A bright, concentrated nucleus dominates the central region, surrounded by a smoother, more diffuse halo. The light distribution appears to be centrally concentrated, becoming fainter with increasing radial distance. The galaxy is somewhat elongated, with a discernible major axis. The color profile suggests a relatively evolved stellar population. The inner regions of the galaxy appear more yellow and red, while the outer regions appear bluer, suggesting ongoing or recent star formation. There are hints of a faint, distorted disc, but the low resolution limits clear identification of spiral arms or prominent dust lanes. The overall structure suggests a galaxy in transition, possibly from a more actively star-forming phase to a quiescent state.
