This galaxy presents a largely smooth and centrally concentrated morphology. It exhibits an elliptical shape, tending towards an intermediate roundness rather than a perfectly circular or elongated form. The galaxy's core appears as a bright, concentrated region exhibiting a yellowish-white hue, potentially indicative of an older stellar population dominating the central regions. Moving outward from the core, the galaxy displays a gradual fading in intensity. A subtle blueish tinge in the outer regions hints at the presence of a younger, hotter stellar population which has a low overall influence. No significant spiral arm structures or dust lanes are visibly discernible. There is no major or minor mergers visible in this image.
