The galaxy presents as a centrally concentrated object with a primarily smooth morphology. The central region exhibits a bright, yellowish-white hue, suggesting an older stellar population. Fainter, reddish tinges extend outwards from the core, possibly indicating ongoing, albeit diminished, star formation activity. There is a slight elongation or cigar shape, suggesting the galaxy may not be perfectly spherical, but it has high degree of circular symmetry. No clear signs of spiral arms or a prominent disk structure are observed, and there's no noticeable evidence of significant recent merger activity. The overall appearance indicates a relatively evolved system with moderate luminosity.
