The galaxy exhibits a generally smooth morphology, with a slightly elliptical shape. The central region displays a high degree of concentration, with a smooth transition to a less luminous, more diffuse outer halo. There is no strong evidence of spiral arm structure. The galaxy's color profile suggests a relatively old stellar population, with a greater abundance of redder stars in the central bulge, and a hint of bluer stars in the extended disk. There is a suggestion of a minor gravitational disturbance in the galaxy, likely caused by a merger. The projected size is roughly 7.8 kpc. Overall, this galaxy is likely a disk galaxy, but with a dominant bulge, indicating its relative old age.