The galaxy presents as an elliptical morphology, with a high degree of central concentration. It appears predominantly smooth in texture, with a lack of readily discernible spiral arm structure or prominent dust lanes. The central region exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward from the center, the color shifts to a slightly bluer tone, suggesting the presence of a younger, though still not particularly vibrant, stellar population. The galaxy shows minimal evidence of significant ongoing star formation or recent merger activity. It is moderately sized and relatively undisturbed in its overall structure.
