The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape appears elliptical, exhibiting a high degree of roundness. There is no clear evidence of spiral arms or a defined disk structure; the light distribution is relatively uniform, decreasing in intensity from the bright central region outwards. The color profile suggests a predominantly older stellar population, displaying a reddish-yellow hue indicative of evolved stars. There is a distinct absence of significant blue regions, suggesting minimal ongoing star formation. No signs of tidal tails, bridges, or other morphological disturbances that would indicate recent or ongoing mergers are visible.
