The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The core region displays a high surface brightness, appearing nearly spheroidal. The color profile is suggestive of an older stellar population, showing a redder hue in the central bulge. There appears to be little to no evidence of distinct spiral arm structures or significant dust lanes; the light appears fairly uniform throughout. There is no visible sign of any major mergers, however, a small disturbance could possibly be present, but it isn't definitive. This galaxy could be considered to be in a relatively quiescent state of star formation and possibly undergoing passive evolution.
