The observed galaxy appears to be an elliptical or lenticular galaxy, displaying a generally smooth, spheroid morphology with a high degree of central concentration. It is characterized by a yellowish-orange hue, suggesting a relatively older stellar population dominated by evolved stars. There is little evidence of distinct spiral arm structure or significant dust lanes. The galaxy exhibits a fairly round shape. Faint wisps or a very slight asymmetry is present, possibly indicating minor tidal interactions or disturbances. Given the overall morphology and colour indices, this galaxy likely has a suppressed star formation rate.
