The galaxy presents as a concentrated, centrally bright object with a relatively smooth, though not perfectly spherical, morphology. There appears to be a slight elongation, deviating from a perfectly circular profile. A distinct bulge is discernible, transitioning into a more diffuse halo or disk component. There is evidence of some internal structure, possibly faint spiral arm segments, exhibiting subtle variations in color and brightness within the outer regions. The galaxy does not show signs of major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out due to the image resolution. Color gradients suggest a slightly redder core, possibly indicating an older stellar population, surrounded by bluer regions, indicative of ongoing star formation. Overall, the galaxy appears to be a relatively massive system undergoing moderate star formation.
