The galaxy presents as a relatively compact object, exhibiting a smooth, diffuse appearance without prominent spiral arms or a well-defined disk structure. The light distribution suggests a centrally concentrated spheroid. Its overall shape appears somewhat elongated, leaning towards a cigar-like morphology rather than perfectly circular. Color gradients are subtle, with a generally blueish hue. No significant morphological disturbances, such as tidal tails or obvious merger remnants, are immediately apparent, but a minor interaction cannot be ruled out. The galaxy exhibits a moderate level of star formation, consistent with a low to moderate specific star formation rate.
