The galaxy presents as an elongated, cigar-shaped structure. It has a smooth, relatively featureless appearance, indicative of an elliptical morphology. There is no discernible spiral arm structure or prominent dust lane evident in this image. The galaxy exhibits a color gradient, appearing bluer in its central regions and becoming redder towards the outer edges. The blue color in the center suggests the presence of some younger, hotter stars in its core, with a low but active rate of star formation. Its apparent magnitude indicates a high luminosity. While the primary structure is a single object, closer inspection reveals minor irregularities in the outer halo, suggesting possible past interactions or minor disturbances. There is no indication of active galactic nuclei activity or a major merger event currently in progress.
