The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge that emits a yellowish hue, suggestive of an older stellar population. Faint disk-like features are possibly present, but not readily apparent. The galaxy's major axis is noticeably greater than its minor axis, indicating a deviation from perfect sphericity. There is no prominent evidence of spiral arms or significant dust lanes. No tidal tails or obvious signs of major merging events are observed, though minor disturbances cannot be entirely ruled out. Given the color and smoothness, this system likely has a relatively low star formation rate for its mass. The estimated size of this galaxy is approximately 7 kpc.
