The galaxy appears as a concentrated, luminous spheroid, exhibiting a high degree of smoothness. Its color profile leans towards the redder end of the spectrum, potentially indicating an older stellar population and/or significant dust obscuration. There is a small amount of asymmetry, possibly indicative of a recent minor merger, though the primary structure is largely undisturbed. A faint secondary object, red in hue, is located nearby. The overall morphology suggests this is a massive, evolved galaxy with suppressed star formation.
