This galaxy presents a largely smooth morphology, suggesting an elliptical classification, though a subtle disk-like structure cannot be entirely ruled out. The central bulge exhibits a bright, concentrated luminosity, indicative of a high stellar density. Moving outward from the center, the luminosity gradually decreases. The overall color profile leans towards the redder end of the spectrum, hinting at an older stellar population with relatively low ongoing star formation. There appears to be little to no evidence of significant mergers or tidal disturbances. The galaxy appears fairly round, with only a slight degree of ellipticity. 
