The galaxy presents as an elongated, disk-shaped structure with a concentrated central bulge. The light distribution within the galaxy is not uniform. The central region exhibits a brighter, yellowish hue, suggesting a population of older stars. Moving outwards from the center, the galaxy gradually fades into a less intense, bluer color, potentially indicating the presence of younger stellar populations in the outer regions. The overall smooth appearance suggests the galaxy is an early-type spiral or lenticular galaxy, with a relatively large mass and small amount of star formation. The galaxy is oriented such that we observe it edge-on or at a high inclination, obscuring detailed spiral arm structure, if present. There may be a slight warping of the galactic plane, suggesting an interaction in the past. The galaxy exhibits a relatively symmetrical profile with a high degree of concentration, and a small degree of star formation.
