The galaxy presents as a somewhat elongated, cigar-shaped structure. It appears to be relatively smooth, lacking prominent spiral arms or a distinct disk. There is a bright central region that suggests a concentration of older stars, possibly a bulge. The galaxy exhibits a bluish hue, particularly at the ends, suggesting the presence of younger, hotter stars and ongoing star formation. There are subtle indications of possible disturbances or minor tidal features, hinting at potential past or ongoing interactions with other galaxies. Overall, it appears to be an elliptical or lenticular galaxy undergoing some level of star formation.
