The galaxy presents a generally smooth, rounded morphology. The light profile appears centrally concentrated with a diffuse halo, suggesting a spheroidal or elliptical classification. There is no visible disk component or prominent spiral arm structure. The central region of the galaxy exhibits a yellowish hue, possibly indicating an older stellar population. A region of bluer color is also detected, which could suggest an area of active star formation. There is evidence of a potential minor disturbance in the galaxy's structure, possibly a small tidal feature or an irregularity in the light distribution which suggests there has been, or is, a minor interaction with another galaxy. 
