The galaxy exhibits a clear disk structure and is oriented edge-on relative to our line of sight. A prominent central bulge is observable, displaying a somewhat elongated morphology. The bulge appears to gradually fade in brightness from the center to the outer edge, suggesting a relatively even distribution of older stars. There is no evidence of strong dust lanes obscuring the central regions. The disk exhibits hints of faint spiral arms and patchy areas of active star formation, which manifest as slightly bluer regions extending outward from the bulge. There is no indication of a recent major merger or tidal disruption. The galaxy does not appear to be strongly interacting with any other nearby galaxies within the field of view. The overall color profile indicates a mix of both young and old stellar populations, but is dominated by older ones.
