The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a relatively smooth and featureless morphology. It presents an overall elliptical shape, leaning towards a slightly elongated form. The galaxy's light profile displays a central bulge that dominates the luminosity, with a notable decrease in brightness towards the outer regions. The color gradient shifts from a more yellow/orange hue at the core to a bluer tint in the outer parts, suggestive of older stellar populations concentrated in the central bulge and more recent, albeit subdued, star formation activity in the outer disk. There seems to be a slight asymmetrical disturbance to the galaxy's structure, indicative of a possible minor interaction with another galactic body or internal dynamic instability. Further, the lack of clearly defined spiral arms reinforces the classification as a transitional form between elliptical and spiral galaxies.
