The galaxy presents a relatively smooth, elliptical morphology. There appears to be a brighter central bulge or core, with luminosity diminishing towards the outer regions. There is a slight asymmetry to the galaxy's overall shape, possibly indicating a minor interaction or disturbance. In terms of color, the galaxy appears generally yellowish, suggesting an older stellar population, but there are also areas of redder hues visible, possibly from either background objects, or regions of on going star formation. No distinct spiral arms or bars are readily apparent. Overall, the system seems to be an intermediate-mass galaxy with a modest star formation rate.
