This galaxy presents an elongated, cigar-shaped morphology. The central bulge exhibits a concentrated brightness, suggestive of a high stellar density, with a yellowish-orange hue, potentially indicating an older stellar population. There is a faint, diffuse disk extending beyond the bulge, showing a bluer tint, which may be indicative of younger stars and ongoing star formation, though at a relatively low rate. There is some evidence of minor disturbances, but no clear indication of recent major merger activity or strong tidal interactions. Overall, the galaxy appears to be a relatively massive system, with characteristics of both elliptical and spiral galaxies, possibly representing an intermediate or transitional stage.
