The galaxy presents a slightly elliptical morphology with a generally smooth appearance, though some features are discernible. A subtle asymmetry is observed, suggesting possible gravitational interaction or internal disturbances. The central region exhibits a higher surface brightness concentration, consistent with a galactic bulge. Faint, diffuse extensions are present, potentially indicating tidal features resulting from a minor merger event or ongoing accretion. The color distribution suggests a diverse stellar population, with bluer regions possibly indicating areas of recent star formation, and redder regions denoting older stellar populations. A small portion of the galaxy is obscured, indicative of a dust lane. Overall, the galaxy appears to be in a dynamic state.
