This galaxy presents as a relatively smooth, elliptical-like structure, with a notable central bulge. The core appears to be a bright, concentrated region, potentially indicating a high density of stars. A fainter disk or halo extends outwards from the central bulge. The galaxy exhibits a noticeable elongation, appearing cigar-shaped. There are indications of some minor disturbances or irregularities in the outer regions, though they are not significant enough to classify this as a major merger. Overall, the light distribution suggests a galaxy in the process of settling into a more stable morphology. The colors are relatively muted. The central regions of the galaxy appear to be redder than the outer regions, indicating an older stellar population.
