The galaxy presents as a slightly elongated, elliptical-like object. It exhibits a diffuse central region with a yellow-gold hue, indicative of an older stellar population. Faint blue concentrations are observed at the periphery of the galaxy, possibly suggesting the presence of younger, hotter stars or regions of ongoing star formation, although this activity appears subdued. There is some irregular light distribution. The galaxy appears relatively smooth with perhaps a minor disturbance visible. No prominent spiral arms or dust lanes are discernible at this resolution.
