The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears fairly uniform, lacking prominent spiral arms or a distinct bar structure. The overall shape is generally round, with only a slight deviation from perfect circularity. There might be some minor disturbances in the outer regions, but these are not substantial enough to classify it as a major merging event. The galaxy's color profile is a mixture of yellow and orange tones. This color suggests a stellar population dominated by older stars, with relatively low current star formation activity. 
