This galaxy presents as a moderately bright object with a discernible elliptical morphology. The core exhibits a concentrated, yellowish luminosity, suggesting an older stellar population. Moving outward from the core, the galaxy displays a fainter, bluer halo, possibly indicative of ongoing star formation in the outer regions.

The galaxy appears generally smooth, with only subtle hints of spiral arm structures or significant dust lanes. There is some visual evidence of minor disturbances in the galaxy's shape, though this is minimal and does not indicate a major ongoing merger event. The overall light distribution suggests a system dominated by intermediate-age stars, with a lower proportion of young, massive stars contributing to the galaxy's color.
