The galaxy presents as a singular, somewhat elliptical object with a smooth, diffuse light distribution. A concentrated central region is apparent, suggestive of a galactic nucleus. The overall color profile appears to be relatively homogenous, leaning towards warmer tones (yellow-red), particularly within the central region. Fainter, diffuse extensions are observable around the bright central region, giving a fuzzy or indistinct edge to the galaxy. No distinct spiral arms, bars, or other morphological features are readily apparent, indicating a relatively smooth structure. There is no clear evidence of any major ongoing merger events, although slight irregularities in the outer regions cannot be ruled out without further data.
