The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse appearance. There is a discernible central bulge that appears brighter and exhibits a yellowish hue, suggesting an older stellar population is dominant in the core. The outer regions of the galaxy exhibit a bluer tint than the core, which may indicate younger stars and ongoing star formation in these regions. The galaxy shows little evidence of spiral arms or a distinct disk structure. There are no obvious signs of major mergers or significant tidal disturbances, although subtle irregularities might be present in the outer regions. The overall morphology suggests the galaxy is an elliptical, likely a fairly massive galaxy with a modest rate of star formation.
