The galaxy appears as a somewhat elongated, centrally concentrated system, likely an elliptical or lenticular type. The core region exhibits a bright, yellowish-white hue suggesting an older stellar population. Moving outward from the core, the light gradually diminishes, with the outer regions displaying a slightly redder tone, indicative of either older stars or dust obscuration. There is a noticeable absence of distinct spiral arms or prominent star-forming regions. The morphology is generally smooth, with a degree of asymmetry apparent. The overall shape is not perfectly circular, appearing slightly cigar-shaped and disturbed. Though no clear signs of merging are directly visible, a mild tidal disturbance cannot be fully ruled out based solely on the image. The galaxy presents a relatively quiescent appearance, indicative of a system with a moderate stellar mass and a relatively low specific star formation rate.
