This galaxy, at a redshift of approximately 0.31, exhibits a generally smooth morphology, appearing largely elliptical in shape. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. There are indications of a faint, diffuse disk-like structure, though the overall form is not a well-defined spiral. The galaxy demonstrates a redder color profile, typical of galaxies with older stellar populations and ongoing though moderate star formation activity. There is evidence of minor disturbances or interactions, suggesting a possible past or ongoing merger event, as indicated by subtle asymmetries in the galaxy's outer regions. These features could be indicative of tidal forces or gravitational interactions with another, smaller object.
