The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge that transitions gradually into a less defined disk. The color profile indicates a significant population of older stars concentrated within the central bulge, appearing more yellow-orange in hue. The outer regions of the disk display a slightly bluer tint, suggestive of more recent star formation activity. There is no definitive evidence of a strong spiral arm structure, though subtle irregularities in the outer disk may indicate nascent arm formation or past gravitational interactions. The galaxy appears relatively isolated; there's no clear indication of a major merger in progress, though minor disturbances might be present. Overall, this galaxy presents a morphology somewhere between a spiral and an elliptical type.
