The galaxy presents as a somewhat elliptical, smooth object, exhibiting a predominantly yellowish-white color, suggesting an older stellar population and reduced star formation activity within the primary body. It lacks any obvious spiral arm structure or distinct morphological features, appearing largely spheroidal and homogenous in form. There are no obvious dust lanes or regions of intense star formation. Overall, the galaxy exhibits a relaxed morphology, and the color suggests that it is not an extremely active star forming galaxy. It appears fairly isolated, with no clear evidence of a major ongoing merger event, though there could be minor tidal disturbances.
