The galaxy presents a generally smooth morphology, with a central, brighter region indicating a possible bulge. The overall shape appears to be an oblate spheroid, though some asymmetry is present. There is evidence of a disk component, indicated by a slight flattening and elongation along one axis. A faint, extended halo or envelope is suspected based on the gradual fading of light intensity outward from the central region. The galaxy's color profile shifts from a yellowish hue in the core, suggesting an older stellar population, to a slightly bluer tinge in the outer disk, which may indicate some ongoing star formation. A minor disturbance or irregularity is noticed towards one end of the disk, which could be evidence of a small tidal interaction, or recent merger with a smaller object.
