The observed galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. It exhibits a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of on-going star formation. There is no clear evidence of spiral arms, dust lanes, or a distinct disk component. The galaxy is nearly circular in projection, and the morphology shows no signs of significant tidal disturbances or ongoing merger activity. The galaxy appears relatively isolated, based on the surrounding field.
