The galaxy presents as a centrally concentrated, luminous object with a generally smooth morphology. Its overall shape appears close to circular, with a high degree of central symmetry. The light distribution suggests a dominant spheroidal component. The core region exhibits a bright, compact concentration of light, likely indicating a dense stellar population or a possible active galactic nucleus. The galaxy does not show strong evidence of spiral arms or a prominent disk structure in the available image resolution. Faint extensions or irregularities in the outer regions suggest possible tidal interactions or past merger events, but these are not distinct. The overall color appears relatively uniform with a slightly blue tint, implying ongoing star formation. Overall, this galaxy appears to be an elliptical galaxy in the process of star formation. 
