The galaxy presents as an elliptical morphology, with a bright, concentrated central bulge exhibiting a smooth luminosity profile. A faint, diffuse halo extends outward from the central region. The color gradient indicates a bluer central region possibly indicative of ongoing star formation or a population of younger stars. The outer halo appears to be redder, which may indicate an older stellar population. There appears to be a slight asymmetry in the halo's shape, possibly due to minor gravitational interactions. There are no obvious spiral arms or disk features evident. Based on the irregularity of the halo there are likely minor disturbances.
