The galaxy presents as a lenticular or early-type spiral, viewed at an oblique angle. Its morphology exhibits a high degree of central concentration with a relatively smooth overall appearance. The central bulge dominates the galaxy's light, appearing bright and slightly yellow. A faint disk component extends outward from the bulge, though distinct spiral arms are not readily apparent. The disk appears somewhat elongated, suggesting a possible cigar shape. There is no strong evidence of ongoing major merging activity or tidal disturbances, though the presence of minor disturbances cannot be fully ruled out. Colors suggest a population of older stars and a relatively low rate of current star formation.
