The galaxy presents as a centrally concentrated object with a generally smooth morphology, though subtle irregularities are observable. It appears to be an elliptical galaxy, although a faint disk component might be present; its color profile suggests the presence of an older stellar population. The light is more concentrated toward the galaxy's center, with the luminosity gradually decreasing toward its outer regions. Some low-level disturbance is visible that may be indicative of a past merger event. There is a small concentration of bluer light in the core of the galaxy, which may be indicative of a small amount of star formation or an active galactic nucleus.