The galaxy presents as a relatively smooth, lenticular-like system, exhibiting a moderate central bulge that transitions into a broader disk component. The bulge displays a yellowish-orange hue, potentially indicative of an older stellar population dominating the region, with less recent star formation. The disk, while not clearly resolved into spiral arms, shows a subtle bluer tinge at its periphery, suggesting the presence of younger, hotter stars. A dust lane is observed, bisecting the galaxy, lending credence to ongoing but low star formation. There are faint disturbances within the disk, indicating a possible minor merger or interaction.
