The galaxy presents a generally smooth morphology, with approximately 6 kpc effective radius. The light is centrally concentrated with an elliptical isophotal shape. The colour profile suggests a relatively old stellar population, with a significant presence of evolved red giant stars dominating the inner regions and a slightly bluer, potentially younger population in the outer regions. There is no clear evidence of spiral arm structure or a prominent disk. There are potential signs of disturbance. There is no apparent bulge or bar structure. Based on the observed color gradients, it is possible there is a moderate amount of on-going star formation.
