The galaxy presents as a centrally concentrated, smooth system with a notable spheroidal morphology. The core exhibits a yellowish hue, suggestive of an older stellar population. Fainter, bluer light extends outward from the central region, implying the existence of a younger stellar population, although star formation appears to be relatively quiescent. There is no evidence of prominent spiral arms or a distinct disk structure; the light distribution is diffuse and relatively uniform. No major disturbances or signs of ongoing mergers are immediately apparent, although minor irregularities cannot be ruled out at this resolution. The overall color and morphology are consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy viewed at a slight angle.
