This galaxy exhibits an elongated, cigar-shaped morphology. Its central bulge appears to be relatively prominent and smooth, suggesting an older stellar population dominates this region. The galaxy displays a gradient in color, with a reddish hue concentrated in the core, transitioning to yellower hues towards the outer edges of the disk. There is no clear evidence of spiral arm structure, but a subtle disk is discernible. Minimal signs of significant ongoing star formation are apparent, based on the smooth color profile and lack of intense blue regions of high star formation. There are no obvious tidal tails or other major distortions that indicate a recent major merger. Minor disturbances may be present.
