The galaxy presents as a relatively smooth, centrally concentrated object with a slight ellipticity. There is a notable lack of distinct spiral arms or a bar structure. The central region exhibits a bright, yellowish hue, suggestive of an older stellar population. The radial color gradient transitions from the yellowish core to a bluer, but still subdued, outer region. There's no strong evidence of active star formation regions, such as HII regions or dust lanes, visually apparent within the image. There are no signs of any major mergers occurring. The overall morphology is consistent with an early-type galaxy.
