The galaxy exhibits a generally smooth morphology, appearing elliptical in shape. A central bulge region is present, displaying a bright, concentrated core with a yellowish-white hue, suggestive of an older stellar population. A flattened disk component surrounds the bulge and the disk appears to be mostly edge on. This disk shows a bluish tint, potentially indicating the presence of younger, hotter stars. There appears to be a faint reddening at the furthest edges of the disk, possibly due to dust. Overall, the galaxy is moderately bright. The light distribution suggests a system without significant ongoing major mergers, although there might be minor internal disturbances present within the disk.
