The galaxy presents as a single, concentrated object with a generally smooth morphology. The light distribution is centrally concentrated, displaying a notable radial gradient in surface brightness. The core region exhibits a yellowish hue, suggestive of an older stellar population. The overall shape is more or less round, with no immediately apparent spiral arm structures or other distinct features indicating a disk-like morphology. There is no evidence of tidal tails, shells, or other obvious signs of recent major mergers or interactions. Faint, diffuse light extends outwards from the central concentration, fading gradually into the background.
