The galaxy presents as a single, relatively smooth object. It exhibits a slightly elliptical shape, with a high degree of central concentration of light. There is some evidence of disk structure. No obvious spiral arms or bars are discernible. The color profile suggests a population of older stars, with a possible, low level of active star formation. There are no signs of a major merger event; however, the slight asymmetry could indicate a minor disturbance. Overall, the galaxy appears to be in a late stage of evolution.
