The galaxy presents an overall smooth morphology, with a centrally concentrated, bright bulge exhibiting a yellowish-orange hue. A faint, disklike structure extends outwards from the bulge, appearing somewhat elongated. The disk displays a bluer color than the bulge, suggesting the presence of a younger stellar population. There are no apparent signs of strong spiral arms, and the disk is rather indistinct. The galaxy's shape leans toward an in-between, not perfectly round, but not cigar-shaped either. There are no obvious signs of any major merging activity, although a minor disturbance or interaction cannot be entirely ruled out due to slight asymmetry in the outer disk region. The high degree of smoothness within the galaxy implies the majority of the structure is featureless.
