The galaxy presents as a somewhat elliptical structure, its light distribution appearing relatively smooth. There is a hint of a central bulge, characterized by a slightly concentrated and warmer colored light, possibly indicative of an older stellar population. The outer regions diffuse outward, the light becoming bluer, suggesting younger stars and potential star formation activity. There does not seem to be any distinct spiral arm structure nor significant tidal disturbances. The galaxy appears to be isolated and unperturbed.
