The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. It exhibits a yellowish-white color, suggesting an older stellar population with lower rates of active star formation. The galaxy appears somewhat elongated, but it appears to fall somewhere between rounded and cigar-shaped. There is no strong evidence of a spiral arm structure or significant dust lanes. There is some suggestion of a minor perturbation in its structure, but no significant evidence of a major merger event. The galaxy appears to be relatively isolated, without any obvious companion galaxies in close proximity.
