This galaxy presents as a lenticular or elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. The light distribution indicates a centrally concentrated bulge, with a gradual decline in luminosity towards the outer regions. The overall shape is elongated, suggesting it is likely viewed at an inclined angle. The galaxy exhibits a yellowish-orange hue, indicative of an older stellar population and reduced ongoing star formation. There is no obvious evidence of significant dust lanes or active star-forming regions within the visible portion of the galaxy.
