The galaxy presents as a relatively smooth, disk-like structure with a central bulge. The overall color gradient suggests a population of older stars dominating the central regions, exhibiting a yellowish-red hue. Fainter, bluer regions are visible throughout the disk, potentially indicating areas of ongoing or recent star formation. The galaxy's shape appears to be elongated, possibly suggesting an elliptical morphology, or a disk seen at an angle. There is no obvious evidence of strong spiral arms, bar structures, or major mergers with other galaxies. Minor irregularities are present, perhaps indicating minor disturbances or interactions.
