The galaxy presents as a generally smooth, elliptical form with a slight elongation. The central region exhibits a concentrated brightness, suggesting a prominent galactic nucleus. The light distribution appears relatively even, with a gradual decrease in luminosity from the core outwards. There is a slight color gradient; the center appears more yellow/gold, transitioning to a redder hue in the outer regions. No distinct spiral arms or features of ongoing major merging events are readily apparent. Slight distortions, potentially indicative of minor interactions, might be present but these are subtle. There appears to be a general lack of intense star formation.
