The galaxy appears as a moderately bright, disk-shaped object with an inclination that shows it nearly edge-on from our perspective. The central bulge exhibits a bright, concentrated luminosity, suggesting a substantial population of older stars. The disk component shows a relatively smooth structure with a faint bluish hue, possibly indicating the presence of younger stars and ongoing star formation, although dust lanes may exist along the central plane, slightly obscuring the light. Overall, the galaxy seems to be of intermediate mass with some evidence of past or present low-level star formation activity. There is no clear indication of any major mergers or tidal disturbances from neighboring galaxies.
