The galaxy presents as an elongated, cigar-shaped structure with a smooth, relatively featureless appearance. The light distribution suggests a concentration toward the center, with luminosity decreasing gradually outward along the major axis. The color profile appears somewhat uniform across the galaxy, with a subtle shift toward redder hues in the outer regions. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology is consistent with an elliptical galaxy, possibly of type E3 or E4, exhibiting a moderate degree of ellipticity. There are no visible signs of active galactic nuclei activity or recent major mergers. The even light distribution and lack of distinct features suggest a quiescent stellar population with relatively low ongoing star formation. Subtle disturbances are observed in the galaxy's morphology, suggesting a minor merger could have occurred in the past.
