The galaxy presents as a relatively small, disk-shaped object with a bright central region. The disk shows subtle color variations suggestive of differing stellar populations or dust lanes. Faint extensions or tidal features may be present, hinting at past or ongoing interactions with other galaxies or a minor disturbance within the galaxy itself. The overall morphology appears somewhat smooth with no distinct spiral arms, although there are hints of some irregularity in the disk structure. Further spectroscopic analysis is needed to confirm the galaxy's composition and internal dynamics.
