The galaxy presents as a somewhat elongated, disk-like structure, observed at a moderate inclination relative to our line of sight. The central bulge appears to be relatively prominent and exhibits a yellowish-white hue, suggesting a population of older stars. The disk component surrounding the bulge shows a bluer coloration, potentially indicative of ongoing star formation within spiral arms. The galaxy exhibits a relatively smooth overall appearance, although subtle asymmetries and minor disturbances are suggested within the disk. There is no indication of a major merger event, although there is some subtle distortion, perhaps a recent minor merger.
