The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. It exhibits a slightly elliptical shape, tending more towards a rounded appearance than a highly elongated one. There is no clear evidence of strong spiral arm structure or a prominent central bar. Subtle disturbances appear visible that may be indicative of minor ongoing or recent interactions or internal dynamics. The color profile suggests a population of older stars, with the galaxy exhibiting a redder hue.
