The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that decreases gradually in surface brightness towards the outer edges. No obvious spiral arm structure or significant dust lanes are discernible. The overall color seems to be yellowish-white, suggesting an older stellar population with lower rates of recent star formation. It appears undisturbed and relatively isolated, with no signs of a major merger event. The morphology leans toward being round, rather than elongated or cigar-shaped. Some minor disturbances might be present, however, the overall impression is that of a relaxed, evolved system.
