The galaxy appears as a concentrated, elliptical structure. Its overall color profile skews towards the redder end of the spectrum, with a central yellowish hue that gradually fades to a more reddish outer region. There are no distinct spiral arms or bar structures visible, suggesting it is an early-type galaxy with a relatively smooth morphology. The galaxy exhibits high central concentration, which is consistent with an elliptical galaxy containing an older stellar population, that is no longer actively forming new stars. Based on its shape, the galaxy appears to be mostly round. Overall, the galaxy doesn't appear to be interacting or merging with another galaxy.
