This galaxy exhibits a relatively smooth and featureless morphology, suggestive of an elliptical or lenticular type. The light is concentrated towards the center, displaying a bright, unresolved nucleus. The overall shape appears elongated, with an approximate aspect ratio of about 2:1, indicating a non-spherical distribution of stellar mass. There's a subtle color gradient from the central region outward, transitioning from a whiter core to a slightly bluer halo. This may indicate ongoing star formation, though at a relatively low rate. There's no visible evidence of spiral arms, bar structures, or major dust lanes. The absence of significant morphological disturbances suggests the system is relatively isolated and not undergoing a major merger event.
