The galaxy presents a generally smooth and rounded morphology. It exhibits a bright, concentrated central bulge which appears a yellowish hue, suggestive of an older stellar population. The overall light distribution is relatively uniform, with a gradual decline in intensity from the core outwards. There's little evidence of spiral arm structure or prominent dust lanes. The outer regions of the galaxy display a more diffuse and less resolved appearance, hinting at a fainter halo or extended envelope of stars. There is no strong indication of ongoing major mergers or significant tidal disturbances. Any asymmetries are minor.
