The galaxy presents a largely smooth morphology. It exhibits a centrally concentrated luminosity profile, with a bright, well-defined core that diffuses outwards into a more extended halo. The color of the core appears to be somewhat yellow-white, suggesting an older stellar population is present. There are no visually distinct spiral arms or prominent dust lanes. The overall shape is mostly rounded, showing a slight deviation towards an elliptical form. There is no obvious evidence of any recent major mergers or significant tidal disturbances.
