The galaxy presents as a fairly luminous object, with an apparent smooth morphology and a generally round shape. There is a slight elongation, but overall it appears close to circular. The central region exhibits a bright, concentrated core, suggesting a substantial bulge component. A subtle color gradient is observed, with a slightly bluer tint in the outer regions compared to the yellower, more central core, potentially indicating ongoing star formation in the disk. No strong spiral arm features or bar structures are discernible from the image. There may be a hint of a faint disk component, but it is largely obscured by the dominant bulge. The overall appearance suggests a galaxy somewhere between a lenticular and an elliptical type, with characteristics leaning towards the early-type side. There is no obvious sign of tidal disturbances or recent merger activity in this image, although minor interactions cannot be ruled out.
