The galaxy appears as a centrally concentrated object, exhibiting an overall elliptical morphology. The core region presents a bright, unresolved appearance, suggesting a concentration of older stellar populations. The color profile appears relatively uniform, with a general trend towards redder hues across the galaxy. There is little evidence of distinct spiral arms or prominent dust lanes. The outer regions of the galaxy fade gradually, without abrupt truncations. No significant morphological disturbances or signs of recent major mergers are evident. Overall, the galaxy is most likely a relatively massive early-type system, exhibiting characteristics consistent with an elliptical or lenticular classification.