The galaxy presents as a centrally concentrated, fairly symmetrical structure with a generally smooth appearance. The color gradient transitions from a yellowish-white core to a reddish-orange hue around the edges. There are no immediately discernible spiral arm features or a prominent disk. The light distribution is relatively uniform, lacking strong evidence of dust lanes or significant star forming regions. The outer edges of the galaxy appear diffuse, suggesting a gradual decline in stellar density with increasing distance from the galactic center. There appears to be a slight disturbance in the symmetry to the left of the core, indicating a possible minor interaction.
