The galaxy presents as a centrally concentrated object with an elliptical morphology. The light distribution appears smooth and relatively featureless, exhibiting a gradual decrease in surface brightness from the core outwards. There is a slight color gradient, with the central region appearing more reddish compared to the outer regions which show a bluer hue. This suggests a population of older stars in the core and the presence of younger, bluer stars in the galactic disk. The overall appearance is consistent with a disk galaxy with a prominent bulge or a lenticular galaxy viewed from a relatively distant redshift. There is no visual evidence of significant ongoing star formation or active galactic nucleus activity. A low rate of star formation is implied by the bluer color of the spiral arms, but it is still rather low. The galaxy does not show signs of any major mergers or tidal disturbances.
