The galaxy presents a predominantly smooth morphology, appearing as a lenticular or possibly elliptical structure. The central bulge exhibits a concentrated, bright, yellowish-white hue, indicative of an older stellar population likely dominated by red giants. Moving outward from the core, the luminosity decreases gradually, transitioning into a fainter, more diffuse halo with a slightly elongated shape. Subtle blue tinges in the outer regions suggest the presence of some younger, hotter stars, although star formation activity appears relatively low overall. The galaxy shows no distinct spiral arm structure or prominent dust lanes. A minor asymmetry is observable in its shape, potentially suggesting a past interaction or minor disturbance.
