The galaxy presents a somewhat smooth morphology. The light distribution is centrally concentrated, suggesting a prominent bulge component. A faint disk is potentially visible extending outward from the bulge, though its features are not well-defined. The galaxy appears to be tilted with respect to our line of sight. The color of the galaxy is generally yellowish, possibly indicating an older stellar population with relatively low star formation activity. No strong spiral arm structure or obvious signs of recent mergers are apparent, however, the potential minor disturbances cannot be ruled out. The overall shape is elongated, but rounded rather than highly elongated or cigar-shaped.
