The galaxy presents as a relatively smooth, lenticular or early-type spiral, appearing elongated in shape. The central bulge region is bright and concentrated, exhibiting a yellowish hue, which may indicate an older stellar population and reduced star formation activity in that region. Extending outward from the bulge, a faint disk is observed, with a subtle blueish tinge towards the edges. The overall smoothness and lack of distinct spiral arms suggests a later stage of galaxy evolution with a possible reduced rate of ongoing star formation throughout the galaxy. There is no obvious presence of any major disturbances or ongoing merger events. The galaxy has a well defined structure with an intact morphology.
