The galaxy presents an overall elliptical morphology, with a relatively smooth light distribution, although some subtle features are discernable. The central region appears brighter and more concentrated, surrounded by a slightly more diffuse halo of light. There is no clear evidence of spiral arm structure or a distinct disk component within the limits of the image resolution. 

There appears to be a degree of disturbance to the main body of the galaxy, indicative of possible interaction or merging activity. Irregularities in the shape and light distribution suggest a recent or ongoing event. The galaxy exhibits a color gradient, with the central regions appearing somewhat bluer than the outer halo. This may imply a younger stellar population or ongoing star formation in the core, relative to the outer regions. The object has an approximate effective radius of 3.5 kpc.
