The galaxy presents as a generally smooth, elliptical morphology, exhibiting a high degree of central concentration. It appears largely spheroidal in shape, with a subtle elongation along its major axis. The core region shows a bright, concentrated luminosity profile. The galaxy appears yellowish-white, suggesting a relatively older stellar population with lower levels of ongoing star formation activity. There is no apparent dust lane or spiral arm structure visible. The galaxy does not show any strong signs of tidal disturbances or ongoing major mergers, though subtle asymmetries could indicate past interactions.
