The galaxy presents as a moderately bright, compact object. Its overall morphology appears to be somewhat irregular, deviating from a perfect elliptical or spiral structure. There is a dominant central bulge, but it shows signs of disturbances and asymmetries. Patches of bluer light suggest possible ongoing star formation within the galaxy, though it is not widespread. These regions of star formation are generally located away from the central region. There are no apparent spiral arms or a well-defined disk. The galaxy exhibits a slight degree of elongation. Based on the observed features, the galaxy appears to be undergoing some form of interaction or disturbance, possibly a minor merger event.
