The galaxy presents as a lenticular or possibly elliptical morphology, exhibiting a smooth, diffuse light distribution, lacking the distinct spiral arm structures characteristic of disk galaxies. The light profile appears elongated, indicating a cigar shape, and is oriented roughly horizontally in the image. The central bulge is subtly brighter and slightly more compact than the surrounding disk. There is a faint blueish hue, most prominent in the disk surrounding the bulge, suggesting some level of ongoing star formation. Overall, the galaxy seems relatively undisturbed, showing no clear evidence of recent major merger activity or significant tidal interactions.
