The galaxy exhibits a generally smooth morphology. The central region presents a concentrated, bright bulge with a yellow-white hue, suggestive of an older stellar population. Moving outwards from the core, there is a subtle transition to a slightly bluer disk component. This outer region displays a mottled appearance, possibly indicating some level of ongoing or recent star formation. The galaxy shows no obvious signs of major mergers or significant tidal disturbances. Its shape appears largely rounded.
