The galaxy presents as a centrally concentrated object with a smooth light distribution. There is a relatively bright, compact core. The galaxy exhibits a moderate degree of ellipticity, appearing more oval than perfectly circular. While there is a hint of structure beyond the central region, distinct spiral arms or other detailed morphological features are not clearly discernible in the image. Color gradients suggest a possible decrease in blue light towards the galaxy's center, potentially indicating an older stellar population in the nuclear region. There is no obvious evidence of ongoing merging activity or significant tidal disturbances. The overall impression is that of a relatively quiescent galaxy, potentially an early-type spiral or elliptical.
