The galaxy appears to be a spiral galaxy with a central bulge that is bright and yellowish. Fainter, bluish features extend outward from the center, suggesting the presence of spiral arms. The arms are not well-defined, giving the galaxy a somewhat flocculent or patchy appearance. The galaxy exhibits a noticeable disk-like structure, though the disk seems partially obscured or disturbed, possibly due to interactions with other galaxies. The overall light distribution suggests a relatively smooth morphology, but hints of irregularities indicate possible ongoing or past merger events. Based on its color, it appears to be comprised of a significant population of older stars, yet some star formation appears to be occurring in the disk, evidenced by the bluish color.
