The galaxy presents an elongated, cigar-like morphology, suggesting an elliptical classification. Its light distribution appears relatively smooth, lacking prominent spiral arm structures or distinct features. The central region exhibits higher luminosity, indicative of a concentrated nucleus. A subtle color gradient is observed, transitioning from bluer hues in the outer regions to slightly redder tones towards the core, potentially indicating differing stellar populations or dust content. Overall, the galaxy appears undisturbed, showing no signs of major mergers or significant tidal interactions.
