The galaxy presents as a relatively compact object. The central region appears to be dominated by a bright, smooth component, suggestive of a galactic bulge. Surrounding this central region, a fainter, more diffuse disk-like structure is observed. There is some irregularity and patchiness within the disk, potentially indicative of star-forming regions or dust lanes. The galaxy appears to be slightly elongated. There might be some signs of tidal disturbances or minor merger activity. There seems to be a faint red emission on the lower left and lower right, possibly dust.