The galaxy presents a generally smooth appearance with a pronounced central bulge. It appears to be an elliptical or lenticular galaxy, potentially viewed edge-on or at a high inclination. The color profile suggests a relatively older stellar population, as indicated by the yellow-red hue of the bulge, with a possible hint of younger, bluer stars within the disk component. The disk appears elongated, exhibiting a cigar-like shape. There are no obvious signs of ongoing major merger activity, though the disk's structure might suggest minor disturbances or past interactions. The overall morphology suggests an evolved system with a substantial stellar mass. Star formation is likely suppressed in the central regions, with a possible low-level of activity occurring in the outer parts of the disk.
