The galaxy presents as a central, concentrated bulge surrounded by a less defined disk. The bulge exhibits a smooth, yellowish hue, indicative of an older stellar population. The disk, appearing larger but less luminous, displays a mottled texture with hints of blue and red, suggestive of ongoing star formation and varying stellar ages. An interaction or merger event is highly suspected, as the galaxy displays irregularities on its right side. This could be a second galactic core or a tidal tail produced during the merger. The galaxy exhibits a moderate degree of roundness. Overall, the galaxy appears to be a massive object with significant star-forming activity, especially within the disk.
