The galaxy presents an elliptical morphology, exhibiting a smooth, largely featureless structure. The central region displays a concentrated, bright yellowish-white luminosity, indicating a significant population of older stars. There is a subtle color gradient moving outwards from the center, transitioning towards a fainter, slightly greenish-yellow hue in the outer regions. This suggests the presence of a younger stellar population or some ongoing star formation, although it appears subdued. There may be some minor disturbances in the outer regions of the galaxy, although this is difficult to assess with complete certainty. Overall, it appears to be a relatively massive galaxy with a modest star formation rate.
