The galaxy presents a relatively smooth morphology, appearing largely elliptical in shape. A central bulge region is discernible, exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer color, potentially indicating the presence of younger, hotter stars and ongoing star formation, although at a relatively low rate. There are no obvious signs of spiral arm structure or a prominent dust lane. Faint, disturbed features can be seen in the surrounding areas of the galaxy. There is a possibility of minor tidal disturbances suggesting a past or ongoing interaction with a companion galaxy, although no clear merger is evident in the image.
