The galaxy presents a relatively smooth morphology, appearing elliptical in shape rather than displaying prominent spiral arms or a well-defined disk structure. Its central region exhibits a concentrated brightness, suggestive of a substantial galactic nucleus. The color profile indicates a mature stellar population, with a bias towards redder wavelengths, implying the presence of older, less massive stars. There's a hint of bluer light in the outer regions, potentially signaling ongoing, albeit subdued, star formation activity. The galaxy shows no major signs of ongoing mergers or significant tidal disturbances, retaining a generally undisturbed appearance. Its overall form leans more towards a roundish shape with a hint of elongation.
