The galaxy presents as a relatively compact object with an overall elliptical morphology. A smooth, centrally concentrated bulge dominates its structure, with a subtle transition towards the outer regions. There is very little observable dust, and star formation appears to be low. There is evidence of a small disturbance in the galaxy's form, which can be seen by a small tail or arc that is coming off of the central bulge on one side. There is no clear sign of ongoing major merger activity, and the color suggests an older stellar population.
