This galaxy appears to be a relatively smooth, elliptical type. It has a centrally concentrated bulge that transitions gradually into a fainter, more diffuse outer halo. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population. There is no obvious spiral structure, prominent dust lanes, or bright star-forming regions visible in this image. The overall shape is moderately round, with no signs of major disturbances or merging activity. A hint of bluer light is visible in the outer regions. The galaxy shows a general lack of distinct features, suggesting a relatively quiescent evolutionary state.
