The galaxy presents as a relatively smooth, disk-shaped object. Its color profile indicates a significant population of older stars, suggested by the yellowish hue concentrated toward the galactic center. The galaxy is elongated, appearing cigar-shaped, and lacks any visually apparent spiral arm structure. There is a faint bluish tinge around the outer edges of the disk, possibly indicating regions of more recent, albeit subdued, star formation. No significant distortions or tidal features are discernible, suggesting the absence of recent major merger events. There are no obvious signs of any strong active galactic nucleus.
