The galaxy presents an elliptical morphology, appearing largely smooth with a high degree of central concentration. The light profile suggests a gradual decline in surface brightness moving outwards from the core, lacking distinct spiral arm features or prominent dust lanes. The core exhibits a yellowish hue, potentially indicative of an older stellar population. Extending outwards, the galaxy's color transitions to a slightly bluer tone, suggesting the presence of some younger stars, although the overall proportion appears less than that in typical spiral galaxies. The axial ratio indicates the galaxy is somewhat elongated, but not dramatically so. There's a subtle indication of some minor asymmetry in the outer regions, possibly hinting at a past minor interaction or disturbance, but the dominant impression is that of a relaxed, relatively undisturbed system.
