The galaxy presents a generally smooth appearance, with a slightly elongated shape that could be described as being somewhere in between round and elliptical. There is a noticeable central bulge that appears brighter and more concentrated than the outer regions. Faint, diffuse extensions are present, but they are not well-defined as spiral arms or distinct features. The color profile suggests a mix of stellar populations, with the central region possibly containing a higher concentration of older, redder stars, and hints of bluer regions. However, the overall color is not strongly suggestive of significant ongoing star formation. Based on these characteristics, it would be classified as a disk galaxy that shows some disturbance.
