The galaxy appears as a centrally concentrated, elliptical-like system. Its morphology is generally smooth, with a notable lack of distinct spiral arms or a prominent disk. The light profile transitions gradually from a bright core to fainter outer regions. The galaxy exhibits a yellowish hue in the center, suggesting an older stellar population dominated by evolved stars. There is some evidence of bluer colors in the outer edges which indicates the presence of some younger stars, or could indicate a more complex stellar population distribution. Although there is no major evidence of interactions with other galaxies, subtle features could be suggestive of minor disturbances or a past merger event. Overall, the galaxy appears to be relatively isolated and mature.
