The galaxy presents as a roughly elliptical structure with a smooth, diffuse light profile. There is no visible evidence of spiral arms or a distinct disk component. The central region exhibits a brighter, more concentrated light distribution, suggestive of a galactic bulge. Color gradients are subtle, with a slightly bluer hue in the outer regions compared to the inner, yellower core. This could indicate ongoing, albeit low-level, star formation in the galaxy's outskirts. The overall morphology suggests a relatively evolved system, potentially an early-type galaxy with a dominant spheroidal component. There are no obvious signs of recent major mergers or tidal disturbances in this image. The galaxy's shape is close to round, not elongated or cigar shaped.
