The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a bright, yellowish core indicative of an older stellar population dominating the central region. A faint, diffuse halo surrounds the core, with colors trending towards redder hues. There is no visible evidence of spiral arms, strong dust lanes, or active star formation regions. A lack of any tidal tails or asymmetries suggests that there have been no major merging events occurring recently. Small disturbances or minor mergers cannot be ruled out, however they would have minimal visibility. The color profile indicates that the galaxy is composed of old stars.
