The galaxy presents as a somewhat symmetrical structure, exhibiting a centrally concentrated luminosity profile. The core region is characterized by a reddish-orange hue, potentially indicative of an older stellar population. Moving outwards from the core, a subtle transition to a bluer color is observed, which may suggest the presence of younger stars or ongoing star formation activity, although not particularly prominent. Faint, diffuse outer regions surround the central component and a spiral arm or other disturbed feature may be present; however, this is not especially distinct. The galaxy appears somewhat smooth in texture, but not perfectly elliptical; the slight asymmetries of the outer regions suggests the possibility of recent or ongoing interaction with another galaxy, or simply a feature rich disk galaxy with many stars and nebulae. The overall morphology of the galaxy does not reveal any particularly strong disturbances but subtle signs of a minor interaction are possible.
