The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a relatively smooth, diffuse structure. It is elongated in shape, displaying an axial ratio indicating a noticeable flattening. The light is dominated by older stellar populations, with a lack of prominent spiral arms or significant dust lanes. There is a suggestion of a bulge component, with a concentration of light towards the galactic center. Overall, the galaxy presents a quiescent and evolved morphology, indicative of lower current star formation activity. There is a slight disturbance to the symmetry, implying a minor interaction with another galaxy may have recently occurred. The color profile leans towards the redder end of the spectrum.
