The galaxy presents a generally smooth morphology, exhibiting characteristics consistent with an elliptical type. The light distribution is concentrated towards the center, displaying a bright core that gradually diminishes in intensity outwards. The overall shape is elongated, resembling a slightly flattened spheroid rather than a perfect sphere or a distinct disk. There is minimal visible evidence of spiral arms or intricate dust lanes. Color gradients suggest a dominant population of older stars, with a reddish hue throughout the main body. Subtle irregularities in the outer regions hint at possible past interactions or minor disturbances, although no major tidal features or ongoing mergers are clearly observed. A hint of blue is observed at the edge of the galaxy, which suggests the presence of younger stars.
