The object presents as a relatively compact, elliptical galaxy, appearing largely smooth and featureless in this imaging. The light profile seems well-described by a Sersic model with a relatively high Sersic index, suggesting a concentrated nucleus and a steep decline in surface brightness with radius. The axial ratio indicates that the galaxy is moderately elliptical in shape. The galaxy appears to be a reddish hue, suggestive of an older stellar population with relatively low ongoing star formation. Overall, the morphology points towards a mature, early-type galaxy.
