The galaxy presents as an elongated, cigar-shaped form. A central bulge appears prominent, displaying a concentrated, yellowish hue, suggesting an older stellar population. Extending outwards from the bulge, a fainter, bluer disk structure is visible. The disk exhibits some level of disturbance or irregularity, with subtle indications of tidal features or ongoing interactions, though no major mergers are immediately obvious. There is evidence of star formation within the disk, indicated by the presence of bluer regions. Overall, the galaxy appears to be relatively massive, with an actively star-forming disk and a substantial, evolved central bulge.
