This galaxy presents a somewhat irregular morphology. There is evidence of a central bulge appearing with a yellow-orange hue, indicative of an older stellar population. The main body of the galaxy extends outwards, showing some features that could be described as a disk, although it lacks distinct spiral arms. The color shifts toward the blue end of the spectrum in these outer regions, potentially indicating regions of active star formation. There appears to be a faint extension on one side, which is suggestive of a minor interaction or tidal feature. Some degree of disturbance is visible within the overall structure, implying it may be in the process of merging or experiencing a tidal event. The galaxy’s smooth component fraction is notable, but the presence of features disrupts what would otherwise be considered a perfectly elliptical appearance.
