The galaxy presents a complex morphology, potentially indicative of an ongoing or recent interaction. It appears to be elongated along a vertical axis, exhibiting an "in-between" roundness, though leaning toward a cigar shape. The light distribution is relatively smooth, with some suggestions of a disk structure in the lower portion. There are signs of possible minor disturbances or tidal features, perhaps evidence of interactions influencing the galaxy's overall form. Some regions appear disturbed and indicate possible merger activity. The color distribution suggests a primarily older stellar population dominating the light output, with a lower contribution from younger, bluer stars. The estimated size indicates it is a moderately sized galaxy.
