The galaxy presents as a moderately inclined disk, exhibiting a generally smooth morphology. Its overall shape is elongated, with a bulge that appears somewhat more luminous than the rest of the galaxy. The central region is dominated by a yellowish hue, suggesting an older stellar population. Fainter blue regions are visible toward the edges of the disk. A possible minor interaction or disturbance is indicated by a tidal tail-like structure emanating from one end of the disk. The galaxy shows a relatively high concentration of light, which suggests that a large portion of the luminosity is contained in the center.