The galaxy presents as a relatively compact, elliptical morphology, with a smooth appearance and no discernible spiral arm structure. The color profile indicates a dominant population of older stars, emitting light primarily in the redder portion of the spectrum, with some contribution in the green band, resulting in an overall yellowish-orange hue. The galaxy exhibits a high degree of central concentration, suggesting a well-developed spheroidal component. There are no obvious signs of recent major mergers or tidal disturbances in the image. The galaxy appears fairly isolated, with no other galaxies in close proximity that would indicate ongoing interactions.
