This galaxy exhibits a generally smooth morphology with an apparent absence of well-defined spiral arms. The galaxy's color gradient indicates the presence of both older stellar populations, particularly towards the central bulge, and regions of recent star formation. The inner region appears yellowish-white, suggesting a dominant population of older stars. Fainter blue hues are visible within a disk-like structure, indicating some level of on-going star formation. The galaxy does not display any obvious signs of a major ongoing merger or tidal disruption; however, there may be a minor disturbance or asymmetry. The overall shape is somewhere between round and elliptical.
