The galaxy presents as a relatively compact object with a central, bright core. The overall color profile indicates a moderately blue hue, suggesting a possible presence of younger stellar populations and ongoing star formation within. The morphology of the galaxy appears somewhat disturbed or irregular, exhibiting a slight asymmetry in its light distribution. A faint, diffuse halo or extended structure may be present, though subtle. Based on the features, the galaxy could potentially be undergoing minor interactions. Further spectral data will be required for confirmation.
