The galaxy presents as a centrally concentrated, luminous object with an overall slightly elliptical morphology. The core exhibits a bright, yellowish-white glow suggestive of an older stellar population. Moving outward from the central bulge, a fainter, bluish halo is visible. This bluer component likely indicates the presence of younger stars and regions of ongoing star formation. The overall structure suggests a disk galaxy, although the disk features are not very well defined or prominent. There are no obvious signs of major interactions or mergers. Minor disturbances cannot be fully ruled out.
