The galaxy presents a predominantly smooth morphology with a subtle, elongated shape. It appears largely undisturbed, lacking significant signs of mergers or tidal features. The color profile suggests a higher concentration of older stellar populations within the central bulge, indicated by the yellowish-orange hue. The galaxy exhibits a relatively low star formation rate, consistent with its evolved stellar populations. There is little evidence of spiral arm structures. Overall, this appears to be a lenticular or elliptical galaxy. 
