The galaxy presents an overall smooth morphology, with a slightly elongated, cigar-shaped appearance. The central region displays a concentrated brightness, suggesting a prominent galactic nucleus. The color profile transitions from a warmer, yellowish hue in the center to cooler, bluish tones in the outer regions. This may indicate older stellar populations in the core, with younger, bluer stars populating the outer disk or halo. A subtle asymmetry in the galaxy's structure could be present, potentially hinting at minor gravitational interactions or internal disturbances. The lack of well-defined spiral arms or a distinct disk structure points towards it being a lenticular or possibly an elliptical galaxy, though some form of disk is likely present. Evidence of ongoing or recent star formation appears limited based on the subtle bluer regions.
