The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, largely featureless morphology. It appears to be disk-like but with a relatively homogenous light distribution, lacking distinct spiral arms. The central region displays a bright, concentrated luminosity, suggesting the presence of a substantial galactic nucleus. 

There is evidence of some disturbance. A faint, diffuse halo surrounds the central region, hinting at possible tidal interactions or past merger events. Color gradients suggest that the galaxy has a moderate rate of star formation. The galaxy exhibits an overall blue-ish hue. The blue tint is consistent with the presence of younger stars, and it suggests the galaxy has a notable amount of recent star formation. The object appears moderately redshifted, indicating a significant distance.
