The galaxy presents as a moderately sized object with an apparent visual magnitude indicating it is relatively faint. The overall morphology suggests a disturbed system. There appears to be a central, somewhat concentrated region, possibly a bulge. However, the dominant characteristic is the presence of significant disturbances and irregularities in its structure. A faint, diffuse halo surrounds the brighter central region, exhibiting a mottled and uneven distribution of light. There is evidence of tidal features or disrupted arms, possibly indicative of an ongoing or recent merger event. The color distribution is not uniform, with subtle variations suggesting differences in stellar populations or dust content throughout the galaxy. Given the structural disturbances, further investigation is warranted to ascertain the nature of the interaction or the cause of the observed distortions.
