The galaxy presents as an elongated, diffuse object with a moderately smooth appearance, appearing generally featureless. It shows a slight deviation from a perfectly circular shape, leaning towards a cigar-shaped morphology. The light distribution is concentrated towards the center, which suggests the presence of a central bulge or core. The galaxy has a bluer hue, which could be due to ongoing star formation. There is evidence of minor internal disturbances, though it is unclear whether this indicates interactions with another galaxy. The overall impression is that of a relatively low-mass galaxy that exhibits a slow rate of star formation.
