The galaxy presents a relatively smooth and amorphous structure, indicative of a likely elliptical or lenticular morphology.  There is a slight elongation, but no discernable spiral arms or prominent disk features are visible. The galaxy displays a moderately concentrated core with a gradual decline in luminosity towards the outer regions. Its color profile appears moderately red, suggestive of an older stellar population with lower ongoing star formation. There are hints of possible minor tidal disturbances or interactions, with a slight asymmetry in the halo. No major mergers or strong tidal tails are apparent. Overall, the galaxy seems like a relatively isolated system undergoing passive evolution. 
