The galaxy exhibits a generally elongated, cigar-shaped morphology. The central region shows a high degree of concentration with a bright, yellowish-white core. This core is suggestive of an older stellar population. Extending outwards from the core, there are diffuse, bluish regions along the major axis. These regions likely contain younger, hotter stars and indicate ongoing or recent star formation. There are no readily apparent spiral arm structures or prominent dust lanes. The overall appearance suggests a galaxy transitioning from a more actively star-forming phase to a more quiescent state. Subtle asymmetries may indicate minor gravitational interactions with neighboring galaxies in the past, but the overall structure is relatively undisturbed. The galaxy appears to be an intermediate-mass system, exhibiting both old and young stellar populations, and possessing signs of a potential evolutionary shift in its star formation activity.
