The galaxy presents as a largely featureless elliptical, exhibiting a smooth, diffuse morphology. The color profile is dominated by reddish-yellow hues, suggesting an older stellar population. The galaxy appears generally rounded, though not perfectly circular. There is no obvious indication of active spiral arms or a prominent central bar structure. The overall light distribution decreases gradually from a bright central region toward the outer edges, with no discernible dust lanes or other significant discontinuities in brightness. There may be a slight asymmetry or minor disturbance to the disk. The galaxy exhibits a relatively low rate of star formation, with most star formation localized to the disk. The galaxy appears to be a single, relaxed system, with no strong signs of recent or ongoing major mergers.
