The galaxy presents as a relatively smooth, elliptical morphology. It appears elongated, with an approximate axis ratio suggesting a classification leaning towards an E4 or E5 on the Hubble scale. The central bulge exhibits a high surface brightness and a yellowish-red color, likely indicative of an older stellar population. The isophotes are generally regular and concentric, showing little evidence of strong tidal interactions or recent mergers. There are no prominent spiral arms or dust lanes visible, further supporting the classification as an elliptical galaxy. There are no obvious knots of star formation present within the galaxy's disk. Overall, the light distribution is centrally concentrated, with a gradual decline in intensity towards the outer regions of the galaxy.
