The galaxy presents as an elliptical morphology with a moderately smooth profile. The core appears to be concentrated and bright, suggesting a relatively high stellar density in that region. The overall color is reddish-yellow, which could indicate an older stellar population with lower rates of active star formation. The galaxy appears elongated, potentially suggestive of a cigar shape. There are no clear signs of spiral arms or prominent dust lanes in the image. No major mergers seem to be occurring but slight disturbances cannot be ruled out. The galaxy is estimated to be around 8.8 kpc in radius, which, along with the mass estimates, suggests that it is a normal mass galaxy. The star formation rates are low, which reinforces the idea that this galaxy is composed of older stars.