The galaxy presents as a single, somewhat diffuse object with an overall elongated shape. The light distribution is uneven. A brighter, more concentrated region appears to be present at one end, fading to a more diffuse extent on the opposite side. There is evidence of multiple knots of light within the galactic body, suggesting regions of concentrated stellar activity or differing stellar populations. The color gradient transitions from a warm, reddish hue in one area to a cooler, slightly bluer tint in others. The lack of sharp features and distinct spiral arm structures indicate a likely elliptical or lenticular morphology, with potential signs of a past or ongoing interaction event that has disrupted the original structure.
