The galaxy exhibits a generally smooth morphology, with a central bulge that appears somewhat prominent and spheroidal. The overall shape is more rounded than elongated. There is a subtle disk component. There is a very minor disturbance present. The color profile suggests a population of older stars, with a noticeable reddish hue emanating from the central region. Star formation appears to be occurring. The galaxy's moderate distance contributes to the blurring of fine details.
