The galaxy presents a generally smooth morphology with a somewhat round appearance. It exhibits a dominant central bulge, which appears to be a concentrated region of older stellar populations, indicated by the redder hue. There is subtle evidence of a surrounding disk structure. The light is relatively uniform throughout, suggesting a lack of significant active star formation in the disk. There are some small disturbances present, possibly suggesting an ongoing or recent minor interaction. The relatively smooth structure implies a well-mixed stellar population within a single structure. Overall, this galaxy appears to be in a fairly settled state.
