The galaxy presents as an elongated, disk-shaped structure viewed nearly edge-on. A prominent central bulge exhibits a smooth, concentrated distribution of light, appearing more yellow in color, suggesting a population of older stars. The disk, extending outwards from the bulge, displays a bluer hue, possibly indicative of ongoing star formation. The disk appears relatively smooth and thin, without any obvious spiral arm structures visible at this resolution. There is no evidence of any significant ongoing mergers or tidal disturbances, although there is some sign of slight disturbance.
