The galaxy presents an overall smooth morphology, exhibiting a structure that is neither strongly spiral nor elliptical. The shape appears elongated, approximating a cigar-like form. A subtle color gradient is observed, with the central region displaying a slightly bluer hue, possibly indicative of younger stellar populations or ongoing star formation, while the periphery shows a tendency towards redder tones, suggesting older, cooler stars. There is a faint hint of a disturbance in the outer regions of the galaxy, though no major merger is apparent. This disturbance is most likely a minor tidal interaction or accretion event. The galaxy exhibits a modest level of star formation, characteristic of a system that has largely ceased its period of peak activity. The overall mass of the galaxy is moderate, placing it within the range of typical galaxies found in the local universe.
