The galaxy presents as a relatively compact object, appearing somewhat amorphous in shape. The light distribution is not uniform; there are distinct clumps of varying color and luminosity scattered throughout the galaxy's main body. A central region exhibits a more concentrated, yellow-orange hue, potentially indicative of an older stellar population. To the side, a bluer region suggests the presence of younger, hotter stars and ongoing star formation. There are hints of structural features, with slight distortions possibly indicating gravitational interaction or recent merger activity. However, the resolution limits a definitive conclusion on the exact morphological classification and the nature of these structures.
