This galaxy exhibits a generally smooth morphology, with a high degree of central concentration of light. The shape is approximately elliptical, though there is an apparent elongation along one axis, suggesting a possible transition between a spherical and more cigar-like structure. The color profile indicates a predominantly older stellar population, as evidenced by the redder hue concentrated in the central bulge. Hints of bluer light in the outer regions suggest the presence of some younger, star-forming regions, but this activity appears subdued. There is no readily apparent evidence of major disturbances or ongoing mergers, with only subtle hints of minor irregularities in the light distribution.
