The galaxy appears to be a relatively smooth, elliptical-like object, possibly a lenticular galaxy at intermediate redshift. The galaxy exhibits a bright, concentrated central bulge that transitions smoothly into a more diffuse halo. The colour profile appears to be relatively homogenous, trending towards redder hues with some faint suggestion of possible dust lanes or substructure in the lower halo. The overall shape is somewhat oblate and the smoothness implies that the object is quite massive and likely contains an older stellar population. There may be some minor tidal interactions or disturbances visible, but the majority of the morphology is smooth and lacks obvious signs of an active merger event. The galaxy appears to be quite red, suggesting either an older population, significant dust extinction, or the effects of redshift. Star formation is likely suppressed.
