The galaxy presents a moderately elongated, cigar-shaped morphology. Its central region appears relatively smooth and featureless, exhibiting a concentrated bulge. A faint, diffuse disk extends outward from the bulge, showing only subtle hints of spiral structure. The color gradient suggests a relatively older stellar population, with a slightly bluer hue in the central bulge transitioning to redder tones in the outer disk. There is no apparent evidence of ongoing major merger activity, although subtle disturbances or tidal features might be present.
