The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, with the light intensity gradually decreasing towards the outer edges. The color profile appears to be somewhat uniform across the galaxy, tending toward a yellowish hue suggestive of an older stellar population. There's a high probability that it's a smooth elliptical galaxy, which is supported by the observed lack of defined spiral arms or significant dust lanes. There is a high probability that it's an elliptical galaxy, which lacks active star formation and would likely show relatively low specific star formation rates. Overall, the galaxy appears relatively undisturbed.