This galaxy presents as a relatively smooth, elliptical form. The light distribution is concentrated towards the center, indicating a prominent bulge. The color profile suggests an older stellar population dominating the core. The overall structure is elongated, verging on a cigar shape. There is a slight hint of a disklike structure, but it is faint. No prominent spiral arms or distinct features are visible. The galaxy is experiencing a relatively low star formation rate. It appears to be a fairly isolated galaxy, showing little evidence of recent or ongoing mergers or significant tidal disturbances.
