The galaxy appears as a diffuse, centrally concentrated object with a generally smooth morphology. There is a slight elongation in its overall shape, deviating from a perfectly circular appearance, tending towards a slightly rounded shape. The galaxy exhibits a color gradient, with a more yellowish-red hue centrally, suggesting an older stellar population. The outer regions appear slightly bluer, hinting at the presence of some younger stars but not a high amount. The object does not show any strong evidence of spiral arm structures or a prominent disk, nor is there obvious signs of tidal disruption.
