The galaxy presents as an elliptical morphology. It is elongated, displaying a relatively smooth light distribution, which appears centrally concentrated with a bulge dominating the luminosity profile. There is no clear evidence of spiral arm structures. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the center, the color transitions to a bluer tint in the outer regions. There is a lack of prominent dust lanes or significant star-forming regions.
