The galaxy appears as a slightly elongated, elliptical structure. It exhibits a smooth morphology, with a concentrated central bulge and a fainter, diffuse halo. The color distribution suggests an older stellar population, as indicated by the yellow-red hue, particularly concentrated in the central bulge. There is minimal evidence of spiral arms or prominent dust lanes, further supporting the assessment of it as a galaxy lacking significant ongoing star formation. The galaxy shows a high degree of central concentration. There are no significant signs of any ongoing merger events.
