The galaxy presents as a somewhat elongated or cigar-shaped structure. The light profile appears relatively smooth, with a concentration of light toward the center that gently tapers off towards the edges. Color gradients are subtle, with a hint of redder hues concentrated in the central region, potentially indicating a population of older stars or dust obscuration. The outer regions exhibit a bluer tinge, possibly signifying the presence of younger stellar populations. There is no clear evidence of spiral arms or a distinct disk structure. No significant signs of tidal disruption or interaction with other galaxies are immediately apparent, although there might be some minor asymmetries or disturbances in the outer envelope.
