The galaxy appears as a centrally concentrated, relatively smooth object with a somewhat elliptical morphology. It exhibits a dominant yellowish hue, suggesting an older stellar population. There is minimal visible structure such as spiral arms or prominent dust lanes. The galaxy's light profile seems to gradually fade from the center outwards, supporting the notion of a large bulge component. There are only minor, if any, visual disturbances to the overall morphology, which would rule out any ongoing major merger activity. A very slight elongation is apparent, giving the appearance of being somewhat 'in between' round and cigar shaped. Overall, the galaxy appears to be a well-formed and relatively undisturbed system.
