The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification or a late-stage spiral with a dominant bulge. The light distribution is centrally concentrated, exhibiting a gradual decline in intensity from the core outwards. The galaxy appears to be generally round, with only subtle deviations from perfect circularity. There is no obvious evidence of strong tidal interactions or major mergers. The galaxy exhibits a color gradient, transitioning from a yellow/orange core to a redder halo. The blue light is minimal, implying that the galaxy is dominated by an older stellar population. There is an indication of low levels of ongoing star formation.
