The galaxy appears to be a relatively compact elliptical or S0 galaxy, exhibiting a smooth, centrally concentrated morphology. It shows a spheroidal structure with a high degree of roundness, lacking any obvious spiral arm features or a distinct disk component. The core region presents a bright, relatively homogeneous distribution of light, suggesting a dense stellar population. The color gradient from the central region to the outer halo is subtle, perhaps indicating a uniformly old stellar population throughout the galaxy with minimal recent star formation. There are no obvious signs of tidal interactions, major mergers, or significant internal disturbances, though slight irregularities in the outer halo can be observed. The object appears relatively isolated in its environment.
