The galaxy presents as a centrally concentrated object with a relatively smooth morphology. There is evidence of a disk structure; however, it is not prominent. The central region is dominated by a bright, somewhat diffuse glow, potentially indicative of an active galactic nucleus or a high concentration of older stars. The outer regions display a fainter, bluer hue, suggesting the presence of younger stellar populations and ongoing star formation. There appears to be a very slight asymmetry. Overall, the galaxy appears to be relatively undisturbed, showing no major signs of a recent merger event.
