The galaxy presents a generally smooth morphology, appearing mostly featureless. The light distribution suggests a concentrated central region, with a gradual fading outward. The overall shape is close to circular, showing minimal elongation. The color profile indicates a dominant yellow-orange hue in the core, likely indicative of an older stellar population. Fainter, bluer colors are observed in the outer regions which may indicate recent star formation. There are no obvious signs of spiral arms or a well-defined disk structure, and no signs of ongoing major mergers or significant tidal disturbances.
