The galaxy presents as a centrally concentrated object with a generally smooth appearance, though exhibiting subtle features suggestive of internal structure. The core region appears bright and somewhat unresolved, emitting strongly in blue wavelengths, indicative of potentially active star formation or the presence of an active galactic nucleus. Extending outwards, the galaxy displays a more diffuse halo. There are hints of asymmetry in the outer regions, with a slight elongation along a particular axis. Two less concentrated luminous areas can be distinguished. The overall color profile suggests a composite stellar population, with both older, redder stars and younger, bluer stars contributing to the galaxy's integrated light. Marginal distortions in the structure suggest possible gravitational interactions with neighboring galaxies.
