The galaxy presents a generally smooth morphology with a slight elongation, appearing somewhat cigar-shaped. A dominant central bulge region is visible, surrounded by a fainter, more diffuse disk. There is no apparent spiral arm structure. The overall color is predominantly bluish-white, suggesting a population of relatively young, hot stars, but the central regions exhibit a slightly yellower hue, which may indicate a population of older stars. There are no indications of recent major mergers or tidal disturbances, and the galaxy appears to be relatively isolated.
