The galaxy presents as a relatively smooth, elliptical-like structure, though it is only slightly cigar-shaped. The light distribution is concentrated toward the center, with a fairly rapid falloff in surface brightness towards the outer edges. The galaxy exhibits a yellowish-white hue throughout, indicative of an older stellar population and suppressed star formation. There are no clearly resolved spiral arm structures or prominent dust lanes visible, suggesting that any spiral features have either been disrupted or were never present. No signs of recent or ongoing major mergers or tidal disturbances are apparent. The galaxy appears isolated and undisturbed.
