The galaxy presents an overall smooth morphology, appearing largely featureless with a dominant, centralized bulge. The light distribution is concentrated towards the core, fading gradually into the outer regions. There is a suggestion of a slight elongation, hinting at a disk component viewed at a shallow angle. A secondary, smaller concentration of light is visible nearby, possibly indicative of a minor interaction or disturbance within the system, with the main bulge appearing mostly undisturbed. The overall color of the galaxy is yellowish, suggesting a population of older stars, with subtle variations in hue that could represent localized regions of ongoing, albeit subdued, star formation. There is no evident spiral structure or prominent dust lanes.