The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, appearing quite round. There is a bright, yellowish core, suggesting a significant population of older stars in the central regions. Moving outward from the core, the light becomes more diffuse, with a subtle color gradient shifting towards slightly bluer hues. This may indicate the presence of younger stellar populations in the outer regions, though the overall color suggests a predominantly evolved stellar population. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy does not appear to be undergoing any major merger events or significant tidal disturbances, presenting a well-defined, relatively undisturbed structure. The estimated size of the galaxy is roughly 8 kiloparsecs in radius.
