The galaxy presents as an elongated structure, roughly cigar-shaped, with a bright, concentrated central bulge. The overall color appears bluish-white, particularly towards the core, suggesting a relatively high population of young, hot stars and ongoing star formation activity.  Faint, diffuse arms or extensions are potentially visible emanating from the central region, though their morphology is not well-defined at this resolution. These extensions may indicate the presence of a disk component. There are no obvious signs of a major merger event or significant tidal disturbances, but subtle asymmetries or minor irregularities in the outer regions could suggest minor interactions or disturbances.
