The galaxy presents as an elliptical or lenticular morphology, exhibiting a relatively smooth and concentrated light profile. It appears to be primarily spheroidal in shape with a hint of a possible disk. There is no strong evidence of spiral arm structure or prominent dust lanes. The galaxy's color is generally yellowish-orange, suggesting a stellar population dominated by older, redder stars with a low ongoing rate of star formation. There are hints of a possible minor disturbance, with asymmetry in the outer regions of the galaxy, though the exact cause is uncertain. The galaxy is relatively isolated with only one other faint object appearing near it. There is no obvious tidal debris or other indications of a recent major merger, though the low resolution makes it difficult to make a definitive assessment. The image is consistent with a galaxy that has undergone significant morphological transformation through internal processes or interactions in its past.
