This galaxy exhibits a mostly smooth morphology, with a high degree of central concentration. The light profile appears to be relatively featureless, lacking prominent spiral arms or a distinct bar structure. The overall shape is somewhat elongated, although it isn't highly flattened. There's little evidence of significant tidal disturbances or ongoing merger activity. The color is primarily yellowish, possibly indicating an older stellar population with suppressed star formation. The absence of strong blue light suggests a limited population of young, massive stars. There is a suggestion of a slight asymmetry, potentially indicative of a minor interaction or internal dynamic process, but further investigation is needed to confirm this.
