The galaxy presents as a relatively smooth, elongated structure. It appears to be an elliptical galaxy, possibly of type E4 or E5, based on its apparent flattening. The galaxy displays a concentrated central bulge that fades gradually outward into a diffuse halo. The color appears to be a yellow-orange hue, suggesting a population of older stars with lower levels of active star formation. There is no clear evidence of spiral arms or significant dust lanes. Based on the lack of distinct features, there appears to be no significant ongoing merger activity or major tidal disturbances affecting the galaxy's morphology.
