The galaxy presents a generally smooth morphology, with a notable absence of defined spiral arms or a strong central bar. The object appears elongated, exhibiting an intermediate ellipticity between a circular and cigar-like shape. There seems to be a notable, bright, and active area in the galaxy. Color gradients are subtle, with a slightly bluer hue concentrated in some regions, possibly indicating ongoing star formation. This is also supported by the presence of a distinct patch of redder emission, suggestive of localized dust or older stellar populations. Despite its overall smooth appearance, subtle disturbances can be observed. There are signs of possible minor interactions or internal asymmetries that might reflect previous accretion events.
