The galaxy presents as a relatively compact structure with a smooth, luminous profile. The morphology appears to be primarily spheroidal, exhibiting high central concentration with a noticeable decrease in luminosity moving outward. The isophotes demonstrate a moderate degree of ellipticity.

Color gradients within the galaxy are apparent, with a bluer central region transitioning towards redder hues in the outer regions. The outer portions show signs of disturbed morphology, and the color indicates that these are areas of higher concentration of older stellar populations. This galaxy may have signs of past or ongoing merger activity or tidal disruption in the form of faint and diffuse asymmetric features. The presence of the blue central region may indicate some amount of active star formation, but could also be caused by the presence of an Active Galactic Nuclei (AGN).
