The galaxy appears to be a relatively smooth, early-type galaxy, most likely an elliptical. It exhibits a concentrated central bulge that gradually fades outward, suggesting a lack of significant star formation. The galaxy appears to be relatively isolated with no obvious signs of interaction, such as tidal tails or distortions. The overall morphology suggests the galaxy has undergone significant evolution, potentially exhausting most of its gas supply. There is a slight elongation present, giving it an intermediate shape between round and cigar-shaped.
