This galaxy presents as a relatively small, disk-shaped structure viewed at a high inclination. A pronounced central bulge is observed, exhibiting a bright, concentrated luminosity. The disk itself appears thin and shows evidence of spiral arm structure, although the resolution limits detailed analysis. The color gradient suggests a population of older stars concentrated in the bulge, with bluer, potentially younger stars populating the disk. There appears to be moderate dust obscuration along the plane of the disk, as evidenced by the slightly redder hue and some apparent irregularities in the light distribution. Faint tidal features are potentially observable, suggesting a minor interaction or disturbance event in the galaxy's past.
