The galaxy presents a generally smooth morphology, appearing largely featureless. It exhibits a centrally concentrated brightness profile, suggesting a dominant bulge component. The overall shape is approximately round, showing minimal elongation or distortion. There is some evidence of color variation within the galaxy, with the central region appearing slightly more yellow, potentially indicating an older stellar population or the presence of dust. There is faint red around the galaxy, indicating possible regions of on going or recent star formation. No distinct spiral arms or bar structures are discernible. The galaxy shows no obvious signs of major tidal disturbances or merging activity, indicating it is likely an isolated system.
