The galaxy presents as a relatively smooth, elliptical structure. Its light profile appears concentrated towards the center, with a noticeable decrease in surface brightness moving outward. The galaxy exhibits a yellowish-white hue throughout its body, indicative of an older stellar population. There are subtle variations in color temperature, with the core potentially exhibiting a slightly warmer signature. No prominent dust lanes or spiral arm structures are discernible. The overall morphology suggests a galaxy undergoing relatively quiescent star formation, possibly at a very low rate, given its color and form. There are no obvious signs of recent merger activity or tidal disturbances.
