The galaxy presents a generally smooth appearance, with a slight elongation along one axis, giving it a cigar-like shape. The overall color is somewhat pale, suggesting a population of older stars. There is a slight color gradient across the galaxy, with the central region appearing more yellow, possibly indicating a higher concentration of older stars or dust. There is no clear evidence of spiral arms or a prominent disk structure. A mild disturbance in the galaxy's morphology cannot be ruled out, but there is no indication of an ongoing major merger. The galaxy exhibits a relatively low rate of star formation. Its estimated size is fairly typical for galaxies.
