The galaxy presents as a moderately luminous, relatively compact object with a noticeable central concentration of light. Its morphology appears largely smooth, lacking prominent spiral arms or a well-defined disk structure. The overall shape is somewhat elliptical, tending towards a flattened spheroid rather than a perfect circle. There is a color gradient visible, with the central region exhibiting a yellowish hue suggesting a population of older stars, while the outer regions show a slight bluer tint, possibly indicating ongoing or recent star formation, although at a comparatively low rate. No signs of major mergers or significant tidal disturbances are apparent in the image. Minor structural peculiarities may be present, but are not distinctly discernible at this resolution.
