The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. It exhibits a roughly elliptical morphology, appearing generally rounded. The color profile suggests a population of older stars, indicated by its redder hue. There is no obvious evidence of spiral arm structures or significant dust lanes within the galaxy's body. There are no signs of any major mergers in the galaxy or any major disturbances. There may be a slight minor disturbance to the galaxy. Based on this analysis, the galaxy is potentially a massive galaxy with a relatively low rate of star formation.