The galaxy exhibits a predominantly smooth morphology with a slight elongation, appearing somewhere between elliptical and lenticular. It displays a central bulge with a yellow-gold hue, suggesting an older stellar population with lower levels of recent star formation. Faint blue tinges can be seen in a small section along its edge, possibly indicating areas of younger, hotter stars. A region to the left of the galaxy appears to have a slightly different color to the rest of the galaxy, indicating a possible interaction or minor disturbance. Overall, the galaxy appears to be relatively massive, exhibiting signs of possible past or minor disturbances but not currently undergoing a major merger event.
