This galaxy presents a morphology consistent with an early-type spiral or lenticular galaxy, seen at a moderate inclination. The central bulge appears dominant and relatively smooth, with a yellowish-white color suggesting an older stellar population. Fainter, bluer regions appear along the periphery of the disk, indicating the presence of younger stars and possibly ongoing star formation, though at a low rate. There is no obvious presence of strong spiral arms. The galaxy exhibits a slightly elongated shape, leaning toward the "cigar" shaped side, but not dramatically so, with no signs of major tidal disturbances or ongoing merging activity are evident. Overall, the galaxy appears well-defined, without significant irregularities.
