The galaxy presents a generally smooth morphology with a dominant central bulge. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. There is a slight asymmetry noted in the overall shape. The main body of the galaxy exhibits a pale reddish-white hue, indicating a population of older stars. An area of faint blue-green tinge is observed along an edge of the galaxy, suggesting potential regions of more recent star formation. A small, distinct, redder object is observed as being very closely associated with the galaxy. It is possible the larger body is undergoing a minor interaction.
