The galaxy appears as a centrally concentrated object with a slightly elliptical shape. Its light is generally smooth in appearance, with a lack of obvious spiral arm structures or prominent dust lanes. The color profile suggests a population of older stars, exhibiting a redder hue overall. The galaxy's edges are diffuse, fading gradually into the background sky. There is no strong evidence of tidal features or ongoing major mergers, however, there is a slight possibility of minor disturbance within the galaxy's structure. The overall morphology suggests it's a galaxy undergoing a low level of star formation.
