The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. There is a general lack of distinct features, such as spiral arms or prominent dust lanes. The color profile suggests an older stellar population, given the yellowish-orange hue. The apparent roundness indicates that it is likely viewed close to face-on, with minimal signs of a significant merger or tidal disruption. While a smooth profile is dominant, there might be faint, diffuse features in the surrounding halo, though these are not sharply defined in the available data. The overall morphology is indicative of an early-type galaxy that has largely exhausted its gas supply and exhibits suppressed star formation activity.
