The galaxy appears to be a relatively compact object, possibly an elliptical or lenticular galaxy, based on its somewhat smooth, centrally concentrated light distribution. There is a bright central region that seems to be spheroidal in shape, which may be an active galactic nucleus. A faint, extended halo is visible around this region, indicating a diffuse distribution of stars or gas. Subtle disturbances or asymmetries are observed in the outer regions of the galaxy, potentially suggesting minor tidal interactions or recent accretion events. The color of the galaxy appears to be slightly bluer in some regions, particularly in the halo, suggesting the presence of younger stellar populations. However, the inner region appears more yellow/red, which could indicate a population of older, redder stars. The galaxy does not exhibit a clearly defined spiral structure or disk-like morphology. Overall, it appears to be a complex system with features indicative of both settled structure and ongoing dynamic processes.
