The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggesting a population of older, redder stars. There is little evidence of distinct spiral arms or active star formation regions within the galaxy. The galaxy appears well-defined, with a gradual decrease in light intensity from the core outwards. Faint blue emissions are visible in a patch on the outer edge of the galaxy, perhaps indication of a more recent star formation event. There appear to be no major distortions or tidal tails visible, suggesting it has not experienced any recent major mergers or interactions.
