The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical or possibly a lenticular galaxy, showing minimal disk-like structure. The central bulge is prominent, exhibiting a yellowish hue, suggesting an older stellar population with lower levels of active star formation. The galaxy's overall color index indicates a relatively red object compared to the other blue galaxies, further supporting the dominance of older stars. There is no clear evidence of significant dust lanes, spiral arms, or ongoing major mergers or disturbances within the galaxy, although there is a very faint, diffuse halo surrounding it.
