The galaxy presents as a relatively compact object with a slightly elongated morphology. It exhibits a primarily red hue, suggesting a population of older stars, but with evidence of bluer regions, possibly indicating more recent star formation. The object appears to be largely smooth, but possible faint disturbances are present. A subtle distortion in the galaxy's overall shape could indicate a minor gravitational interaction. Overall, the object appears to be a non-major merging galaxy with very little star formation activity. 
