The galaxy presents as a centrally concentrated elliptical. It exhibits a smooth, fairly regular morphology, with no apparent spiral arms or significant dust lanes visible in this imagery. The light distribution appears relatively uniform, decreasing in intensity from a bright, somewhat diffuse core outwards. The galaxy appears approximately circular, with a slight suggestion of ellipticity. There is no obvious sign of tidal features, shells, or other indications of recent major merger activity. Based on the color gradient, there appears to be an older stellar population dominating the light output, suggesting relatively low ongoing star formation. 
