The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge with a radial falloff in surface brightness. The galaxy is characterized by a slightly elongated, spheroidal shape. There is a hint of a disk like structure, but the overall light distribution is dominated by the central bulge. The core of the galaxy presents a yellowish-white hue, suggesting a population of older stars. Moving outwards, the galaxy appears bluer, likely indicating the presence of a younger stellar population. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances, but some minor disturbances could be present. Overall, the galaxy presents as a relatively undisturbed elliptical galaxy with a mix of stellar populations. The galaxy is relatively small. Star formation appears to be occurring at a fairly low rate. The mass of the galaxy is estimated to be around 10^10 solar masses.
