The galaxy presents a primarily smooth morphology, with a concentrated central bulge exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. Surrounding the bulge is a fainter, more diffuse disk-like structure. The disk component shows hints of bluer colors, suggesting the presence of some younger stars or ongoing star formation, although the activity appears relatively low. The galaxy exhibits an intermediate degree of roundness, not perfectly spherical, yet not highly elongated. There's no obvious evidence of strong tidal features or a major ongoing merger. A subtle asymmetry is observed in the outer disk, potentially caused by a minor interaction or internal dynamics.
