The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The light distribution suggests an elliptical shape, though it deviates slightly from perfect circularity. There is a lack of defined spiral arms or prominent disk structures. The color profile suggests a population of relatively older stars, based on the redder hue observed. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. Subtle, minor asymmetries could be present, hinting at past or ongoing interactions, but these are not immediately obvious. The light is fairly evenly distributed, implying that this is not an actively star forming galaxy. 
