The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's appearance, exhibiting a yellowish hue. The light gradually diffuses outwards from the core, transitioning to a reddish color and then into a bluish halo. The color is consistent with an older stellar population. No distinct spiral arms or prominent dust lanes are discernible within the image, further supporting its classification as an elliptical galaxy. There are no signs of significant tidal disturbances or ongoing major merger events. Faint irregularities in the outer regions may indicate minor interactions or past accretion events. The structure of this galaxy is fairly round and smooth, with little deviation from rotational symmetry. Based on the limited color data, this galaxy has a very low ongoing star formation rate.