This galaxy exhibits a generally smooth morphology. Its shape is elongated, appearing somewhat cigar-shaped rather than perfectly round. The central region displays a higher surface brightness, suggesting a concentration of stellar populations or possibly an active galactic nucleus. There is a subtle color gradient observed, with the central region exhibiting a slightly redder hue compared to the outer regions, which appear bluer. This may indicate older stellar populations in the core and younger, hotter stars in the outer regions. There appears to be a slight warping of the galaxy, and possible signs of tidal disruption occurring. This is only a subtle feature, further investigation is needed. Evidence of minor disturbances is present but further observation and multi-wavelength data may be necessary to confirm the nature of these potential interactions.
