The galaxy appears as an elongated, somewhat spindle-shaped structure. It is roughly oriented along its major axis in the image. The light is concentrated toward the center, suggesting a central bulge or core region. The galaxy exhibits a smooth texture overall, with a subtle change in luminosity from the center outwards. There is an indication of a very faint, diffuse disk surrounding the core. The light emitted is mostly in the green to blue spectrum, suggesting younger stars or active star formation. There is no clear evidence of spiral arms or strong bar structure. The overall structure of the galaxy appears relatively undisturbed, without major signs of tidal interactions or mergers. However, there is a slight asymmetry to the outer region of the galaxy, warranting further investigation into potential minor disturbances. Based on the morphology alone, this galaxy may be classified as an early-type spiral, or potentially a lenticular galaxy.
