The galaxy appears as a small, relatively smooth and compact elliptical galaxy, exhibiting a slight elongation. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. The color profile suggests an older stellar population, as indicated by the yellowish hue. There is no apparent dust lane, spiral arm structure, or active star-forming region visible within the galaxy. Based on its color and morphology, the galaxy is likely a spheroidal system with minimal ongoing star formation. There are no signs of any significant tidal distortions or ongoing merger events.
