The galaxy presents a generally smooth, elliptical morphology with a relatively high degree of central concentration. The light profile suggests a bulge-dominated system with a faint, diffuse halo. The color appears to be fairly uniform across the galaxy, with a tendency toward redder hues, indicative of an older stellar population. There is no distinct evidence of spiral arms or active star formation regions. The galaxy exhibits a slight elongation, and appears to have a relatively undisturbed structure.
