The galaxy appears as a centrally concentrated spheroid of light. The central region exhibits a bright, yellowish-white hue, indicative of an older stellar population. The luminosity gradually decreases with radial distance from the center, transitioning to a faint reddish-orange color in the outer regions. There's a notable absence of well-defined spiral arms or a prominent disk structure, suggesting a relatively smooth morphology. No signs of active star formation are visually apparent, based on the subdued bluish tones. Overall, the galaxy exhibits a generally elliptical or lenticular form, consistent with a more evolved system.
