The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decline in surface brightness towards the outer regions, suggesting an older stellar population is dominant. There is a slight elongation, deviating from a perfectly circular shape. The color profile indicates a redder hue overall, which typically corresponds to a reduced rate of star formation within the galaxy. There is a second object of a similar color nearby, but there is no visible indication of interaction or tidal features disrupting the smooth structure of the main galaxy.
