The galaxy presents an elliptical morphology, exhibiting a smooth and somewhat diffuse luminosity profile. It shows a concentrated central bulge region, characterized by a bright, bluish core. The outer regions display a fainter, greenish hue fading into the background. There is some evidence of minor disturbances to the galaxy's structure, possibly due to a past minor merger event or tidal interactions. The shape exhibits an asymmetry that is suggestive of a possible ongoing interaction. However, a smooth classification is more likely, suggesting a settled state despite potential faint disturbances. Overall the galaxy appears to be relatively quiescent, consistent with a lack of significant star formation activity in the observed bands.
