This galaxy presents as a centrally concentrated object with an overall smooth morphology, though with some notable substructure. The primary body of the galaxy exhibits a luminosity gradient, peaking at a bright, yellowish-white core. This core appears well-defined.

Extending from the main body, there is a distinct reddish component. This feature is spatially separated from the central core and appears as a somewhat irregular formation. It presents an area of intense red-shifted light, suggesting either a region of significant dust obscuration or a population of older stars. 

Given the overall smooth appearance of the galaxy, it can be classified as an elliptical galaxy or a lenticular galaxy, but a potential merger event cannot be discounted. The presence of the secondary, reddish component may be indicative of such an event or a significant region of star formation.
