The galaxy exhibits an elliptical morphology, appearing relatively smooth with a high degree of central concentration. The light distribution suggests that the galaxy is viewed at an oblique angle, as it appears elongated, with a major axis of approximately 11 arcseconds. The bulge dominates the structure of the galaxy. There is no strong evidence of spiral arms or a prominent disk-like structure. Color gradients are subtle, with a slightly redder hue towards the central region and a bluer tint in the outer regions. The smooth appearance and redder color indicates that the galaxy is not forming many new stars, and may be dominated by older populations of stars. There are a few faint patches of diffuse emission within the galaxy, although they are not obviously star-forming regions. The overall structure suggests the galaxy has undergone mergers or interactions, although it is not presently experiencing a major merger event. It is likely a passive or quiescent galaxy with a small amount of residual star formation.
