The galaxy presents a generally smooth, elliptical morphology, exhibiting a fairly even distribution of light across its visible extent. It appears elongated, with a cigar-like shape, suggesting a potential classification along the lines of an E4-E7 galaxy on the Hubble sequence. There is a very slight indication of a disk structure. The galaxy's color profile is complex with some central concentrations of light with a blue-white hue, possibly indicating ongoing star formation, while the outer regions show slightly redder tints indicative of an older stellar population. There's no readily apparent evidence of strong tidal interactions or major mergers. Possible minor disturbances cannot be ruled out based on this image alone.
