The galaxy presents a generally smooth, elliptical morphology. It appears primarily as a spheroidal system dominated by an older stellar population, exhibiting a yellow-reddish hue concentrated towards the center. The central bulge is prominent and appears densely populated. There may be a very faint, diffuse disk component. There is no evidence of strong tidal features or major merger events. The galaxy exhibits a moderate level of star formation activity. The overall structure suggests a galaxy that has largely exhausted its supply of gas for active star formation. The galaxy appears relatively isolated.
