The galaxy presents as a relatively smooth and rounded structure. It appears to be an elliptical galaxy, exhibiting a high degree of central concentration. The color profile is somewhat uniform across the galaxy's body, with a slight concentration of redder hues towards the central region. This color suggests an older stellar population. There is little evidence of spiral arms, dust lanes, or active star formation. The galaxy appears undisturbed, with no signs of tidal tails or ongoing mergers. The overall morphology suggests a galaxy that has undergone significant evolution, likely with minimal current star formation. The estimated size is approximately 3.5 kpc.
