The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears largely smooth in texture, with a concentrated central bulge. The color profile indicates a relatively older stellar population. The central region exhibits a yellowish-orange hue, suggesting a concentration of evolved stars. The outer edges fade into a slightly bluer tint, hinting at the possibility of some ongoing, albeit limited, star formation within the galaxy's disk. The image does not reveal any prominent spiral arm structures or significant dust lanes. There is no apparent tidal distortion or evidence of recent merger activity. The overall structure suggests a galaxy that has largely ceased active star formation, settling into a relatively quiescent state.
