The galaxy presents a generally elliptical morphology, appearing largely smooth and featureless. The central region exhibits a bright, concentrated luminosity profile, suggesting a substantial stellar population. There is a gradual decline in brightness moving outwards from the core. The color appears to be somewhat redder or yellower, indicating an older stellar population and a relatively low rate of ongoing star formation. Some minor disturbances or faint features cannot be entirely ruled out, but overall, the galaxy appears to be a well-defined, relatively undisturbed system. Its roundness is more akin to a sphere, not a cigar shape. There is no strong indication of any major ongoing merger events.
