The galaxy presents as an elongated, likely elliptical, structure. Its light profile appears relatively smooth and diffuse, with no readily discernible spiral arms or prominent dust lanes. The central region exhibits a slightly brighter and more concentrated luminosity, suggesting the presence of a nucleus or central bulge. The overall color appears relatively uniform across the galaxy, with a slightly redder hue, indicative of an older stellar population and lower levels of ongoing star formation. There are hints of a very minor disturbance in the galaxy's morphology, but overall the galaxy does not seem to be undergoing a major merger.
