The galaxy appears to be an elliptical galaxy, showing a smooth, centrally concentrated light distribution. There is a noticeable elongation, suggesting it is not perfectly spherical, with an axis ratio of approximately 0.66. The galaxy exhibits a reddish-yellow hue, consistent with an older stellar population. There is no indication of spiral arms or significant dust lanes. The concentration of light increases toward the center, consistent with a Sersic profile. There is evidence of a merger between two galaxies that have not yet fully coalesced.
