The galaxy presents an elliptical morphology, appearing generally smooth and somewhat elongated. The light distribution is concentrated towards the center, exhibiting a bright, yellowish core indicative of an older stellar population. The outer regions display a gradual decrease in luminosity, transitioning to a fainter, less defined halo. A subtle disk-like feature may be present but this is difficult to confirm. There is no strong evidence of prominent spiral arms or significant dust lanes. Some indications of minor disturbances present. The overall color suggests a relatively low star formation rate. The galaxy does not appear to be undergoing any major merging events, though minor tidal interactions can't be ruled out.
