The galaxy appears as a flattened, elliptical structure, viewed at an oblique angle. Its color profile indicates an older stellar population, with a dominant reddish-yellow hue in its central region. A faint, greenish disk surrounds the core. The structure is smooth and lacks distinct spiral arms or prominent dust lanes, suggesting a relatively quiescent state of star formation. There is only a slight suggestion of tidal interaction or morphological disturbance. It seems to be generally smooth and not actively merging with other objects, or having a high rate of star formation.