The galaxy presents as a slightly elongated spheroid with a concentrated central bulge. The core region exhibits a yellowish hue, which possibly suggests an older stellar population. The overall color of the galaxy appears to be redder as opposed to blue, indicating a dominant population of older stars. It appears relatively smooth, lacking any prominent spiral arm structures or significant dust lanes. There is very slight evidence of a disk. The galaxy seems relatively isolated, with no obvious signs of ongoing major mergers or tidal disturbances. It appears to be undergoing a low rate of star formation.
