The galaxy appears as a single, relatively smooth object with a concentrated central bulge. The primary color of the galaxy is a yellowish-orange hue, potentially indicative of an older stellar population. There is a very faint bluish tinge visible in what might be a very compact disk surrounding the bulge, although this is indistinct. A minor disturbance or tidal feature may be present in the lower left quadrant. The object displays a high degree of roundness in its overall form, with no evidence of significant elongation or bar structures. Merging activity is unlikely but cannot be completely ruled out based on the faint disturbance, though it is more likely that the galaxy is simply tidally interacting.
