The galaxy appears as a somewhat elongated, lenticular or early-type spiral galaxy with a smooth, centrally concentrated bulge. The disk is faint and subtle, exhibiting only a slight hint of spiral structure, possibly indicating an older stellar population with reduced star formation. There is a slight asymmetry observed in the outer regions of the galaxy, hinting at a possible past minor merger or tidal interaction. The galaxy possesses a redder color profile, indicative of a lack of significant recent star formation and suggesting a population of older, redder stars. The overall morphology is relatively undisturbed, with no prominent tidal tails or other signs of major disturbances.
