The galaxy appears as a central, roughly elliptical, luminous object. Its light distribution suggests a dominant bulge component, with a concentration of older stellar populations towards the center, as indicated by its color profile, trending slightly redder. There is a hint of a possible disk structure, though less prominent, appearing slightly elongated. The overall structure is somewhat disturbed; there may be a minor gravitational interaction occurring, as suggested by a slight asymmetry in its shape. There does not appear to be evidence of an active galactic nucleus, and a smooth morphology is the dominant feature.
