The galaxy presents a roughly elliptical morphology, appearing elongated with a cigar-like shape. It exhibits a smooth, diffuse light distribution, suggesting a relatively homogenous stellar population. The core region appears brighter and more concentrated than the outer regions.  A subtle color gradient is observed across the galaxy, with the central region trending toward yellow-orange hues, potentially indicative of an older stellar population and reduced star formation activity, while the outer regions exhibit slightly bluer tones, suggesting a potential for small amounts of ongoing star formation. There is some slight distortion of the light in the form of some fuzzy patches, suggesting possible minor gravitational disturbance, but no clear signs of ongoing major mergers. Overall, the galaxy gives the impression of a mature system.
