The galaxy appears to be relatively small, exhibiting a concentrated central bulge with an elongated morphology. Its shape is more rounded than cigar-shaped, but not perfectly circular. The light distribution indicates a predominantly smooth structure, though subtle irregularities suggest the potential presence of faint, diffuse features within the disk. There is no strong indication of any major ongoing merger activity, although very faint disturbances may be present. The color gradient reveals a slightly redder hue in the central region, indicative of an older stellar population, transitioning to a subtly bluer tone in the outer regions. This may be due to the presence of younger stars in the outer regions. Overall, the galaxy presents a somewhat featureless appearance suggesting a quiescent state.
