This galaxy presents as a relatively small, elongated structure with a high degree of inclination, appearing nearly edge-on from our vantage point. The central region exhibits a significantly brighter, concentrated luminosity, suggesting a prominent galactic bulge. The bulge appears smoothly distributed with a rounded appearance. Extending outwards from this central bulge, a fainter, more diffuse disk is discernible. The disk appears relatively uniform in color, with minimal visible dust lanes or distinct spiral arm structures. The overall color gradient shifts from a yellowish hue in the central bulge to a slightly bluer tint toward the outer edges of the disk, suggestive of younger stellar populations in the outer regions. No major distortions or tidal features are apparent, indicating that the galaxy is relatively undisturbed by major merging events. Overall, the galaxy appears to be a relatively quiescent system with moderate star formation activity.
