The galaxy exhibits a smooth, centrally concentrated morphology. Its overall shape appears elliptical, trending towards an elongated, though not significantly cigar-shaped, form. The color profile suggests a relatively older stellar population with a dominant reddish-yellow hue in the central regions, which fades towards the outer edges. There are no discernible spiral arms or prominent dust lanes. No signs of major mergers are visible, although there is possibly a faint hint of tidal disturbance in the outer regions. Overall the galaxy appears to be a fairly massive quiescent system with a low star formation rate.
