The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated central bulge and a relatively diffuse halo. The orientation suggests a viewing angle that is not face-on, instead the galaxy is being viewed at an oblique angle, presenting an elongated profile. The central region displays a yellow-orange hue, suggestive of an older stellar population. The outer regions show a slight shift towards bluer colors, which could indicate the presence of younger stars. The overall luminosity profile is relatively smooth, lacking the distinct spiral arm features. There are no obvious signs of strong tidal interactions or recent merger events within the immediate vicinity of the galaxy. The galaxy appears relatively isolated.
