The galaxy presents a predominantly smooth morphology, with a centrally concentrated bulge region that appears bright and largely featureless. This central region exhibits a slightly elliptical shape. Fainter, diffuse light extends outwards from the bulge, suggesting a possible disk component, although distinct spiral arms are not readily apparent. There appears to be a subtle asymmetry to the galaxy's overall light distribution, possibly indicating a minor interaction or disturbance. The galaxy displays a color gradient, with the central bulge appearing bluer and the outer regions trending towards redder hues. This color variation is suggestive of ongoing or recent star formation in the central region, while the outer regions may contain an older stellar population. The galaxy is relatively compact, with no obvious tidal features or extended halos. The light profile seems to indicate a slight elongation or flattened disk structure.
