This galaxy presents as a single, largely featureless object. Its light is concentrated in a roughly circular morphology, indicating a possible elliptical classification. The galaxy displays a color gradient, appearing brighter and redder towards its center, with the outer edges exhibiting a slightly bluer hue. This color variation suggests a potential age gradient in the stellar populations, where older, redder stars dominate the core, and younger, bluer stars may be more prevalent in the outskirts. The overall smoothness and dominant central concentration imply minimal ongoing star formation activity, consistent with a more evolved system. There is no clear evidence of spiral arms or a prominent disk structure. The lack of significant tidal features or distortions suggests the absence of recent major merger events, although the subtle bluer outer regions could hint at minor accretion or interactions. The morphology appears relatively undisturbed, supporting the possibility of a dynamically relaxed system.
