The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The galaxy exhibits a yellowish hue, indicative of a population of older stars. There is little evidence of significant star formation within the galaxy, consistent with a red and dead or quiescent system. The apparent roundness of the galaxy suggests it is not highly inclined with respect to our line of sight. No prominent features, such as spiral arms or tidal tails, are visible, implying it has not undergone a major merger recently and is undisturbed. There may be some minor disturbances to the disk, but it is unclear. Overall, this galaxy appears to be a mature, relatively massive system with a suppressed star formation rate.
