The galaxy presents an elongated morphology, displaying a moderate ellipticity. The central region exhibits a relatively smooth texture, indicative of a concentrated stellar population. A faint, diffuse disk-like structure appears to extend from the central region. There is a slight suggestion of a possible tidal tail or other gravitational disturbance, but it is very minor. Overall the galaxy appears to be relatively undisturbed. The color distribution suggests that the nucleus and bulge region may be composed of older stars, while the surrounding area could contain areas of more recent star formation. There is no strong evidence of active galactic nuclei activity based solely on this image.
