The galaxy presents as a moderately luminous object with a distinct, elongated morphology. Its overall color profile suggests an older stellar population with a dominant yellowish-orange hue. The galaxy exhibits a smooth appearance, with limited evidence of spiral arm structures or prominent star-forming regions. A slight central bulge is visible, contributing to the overall elliptical shape. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers. The elongated shape indicates a possible transition from a more rounded system to a cigar shape, suggesting a non-negligible rotational component with some degree of intrinsic ellipticity. Overall, the galaxy appears to be a relatively massive, evolved system with limited ongoing star formation.
