The galaxy presents a morphology consistent with a late-stage spiral or early elliptical type. The central bulge is prominent, exhibiting a concentrated luminosity gradient suggesting an older stellar population. A faint, diffuse disk surrounds the bulge, showing some irregularities. The color profile indicates a bluer hue in the outer regions, potentially indicative of ongoing star formation. While the overall shape appears somewhat rounded, subtle asymmetries suggest possible gravitational interactions or minor disturbances. There is no evidence of a major ongoing merger.
