The galaxy presents as a single, largely homogenous object with no distinct spiral arms or bar structure immediately visible. It exhibits a smooth, elliptical morphology, appearing nearly circular in projection. The color profile suggests an older stellar population, with a yellow-red hue dominating. There is a slight gradient in color and brightness from the core outwards, suggesting a denser stellar distribution towards the center. Marginal irregularities in the outer regions may indicate minor tidal interactions or ongoing accretion events, but the overall structure appears relatively undisturbed. Star formation appears to be largely quiescent.
