The galaxy presents a primarily smooth morphology, appearing rather rounded in shape. A slight asymmetry suggests possible disturbances or ongoing gravitational interactions. The dominant color is a yellow-orange hue, indicative of an older stellar population and reduced recent star formation activity. The galaxy's overall structure lacks prominent spiral arms or a well-defined disk. There is an indication of a central concentration of light, possibly a bulge, surrounded by a more diffuse halo or envelope.
