The galaxy presents as a relatively small, lenticular-like structure, exhibiting a smooth and featureless morphology. Its overall shape appears to be moderately elongated, leaning toward a cigar-like shape. There is no visible evidence of prominent spiral arms or significant dust lanes. The color profile suggests a population of older stars, exhibiting a faint red hue. There is a subtle central bulge region that is brighter than the surrounding disk, but it's not highly pronounced. No signs of major disturbances or mergers are apparent.
