The galaxy presents a generally elliptical morphology. A bright, concentrated central bulge dominates the structure, emitting strongly in yellow-white wavelengths, suggesting an older stellar population. Fainter, more diffuse regions extend outwards from the core in a flattened disc-like structure. The galaxy exhibits some indications of tidal disturbances or merger activity, displaying an irregular outer shape. This may also be indicative of interactions. Faint blueish knots are observed which suggests recent star formation activity is present within the disk. The overall color profile indicates a mix of stellar populations, with the bulge appearing significantly redder compared to the bluer outskirts.
