The galaxy presents a largely smooth morphology, with a high degree of central concentration. There is a lack of distinct spiral arm structures or prominent features indicative of ongoing major mergers or tidal disturbances. The galaxy appears relatively round in shape, with a slightly elongated form. Color gradients suggest an aging stellar population, with a higher concentration of redder stars towards the central regions. There may be a small degree of star formation within the galaxy, but overall, it does not appear to be vigorously star-forming.
