The galaxy presents as an object with a relatively smooth central bulge region, exhibiting a diffuse, extended halo. There is evidence of disk-like features, though they appear somewhat disturbed or irregular, rather than exhibiting a clear spiral structure. A faint blueish haze surrounds the central region of the galaxy. The core appears reddish, indicative of an older stellar population. There may be some indication of interactions or tidal disturbances in the outer regions, potentially indicating a past or ongoing merger event, though it is difficult to make a definite classification without higher resolution data. There is a smaller object that may be another galaxy or some part of this same one. The galaxy appears to be intermediate in terms of its overall morphology, not a pure elliptical, nor a well-defined spiral galaxy. It may be an intermediate spiral or peculiar galaxy.
