The galaxy presents as an elongated, cigar-shaped morphology. There is evidence of a relatively smooth central bulge or core, brighter and more concentrated than the surrounding structure. A faint disk appears to extend horizontally from the core. Subtle distortions and minor disturbances are visible in the outer regions. The color gradient transitions from a bluer hue towards the core to a redder hue in the outer regions. A slightly off-center condensation of light, appearing as a bright spot, may indicate a region of increased star formation. The galaxy also may be in the midst of a minor merger, with some slight disturbances in its structure.
