The galaxy appears as a somewhat smooth object, exhibiting a relatively low level of internal structure. It appears somewhat flattened and elongated with a cigar-like shape. There is no distinct spiral arm structure visible. The galaxy exhibits a redder hue, suggesting a population of older stars. No merging features or major disturbances are clearly observed, although some minor disturbance may be present. The galaxy's size appears relatively compact. The light emitted by the galaxy indicates a relatively low rate of ongoing star formation.
