The galaxy presents an elongated, cigar-shaped morphology. A concentrated, bright central bulge dominates the structure, appearing approximately yellow-orange. This suggests an older stellar population within the core. Fainter, bluer hues extend outwards from the central region, forming a flattened disk. These areas potentially indicate regions of more recent or ongoing star formation. Some subtle irregularities are apparent in the outer disk, potentially due to minor gravitational interactions or internal dynamics. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy, though with some features suggestive of a possible spiral or lenticular type. It is likely undergoing relatively low levels of star formation and is fairly massive. 
