The galaxy presents as a somewhat smooth, rounded object with a concentrated central bulge that emits primarily yellowish-orange light. There is some evidence of a slightly more diffuse, bluer halo surrounding the central region, though the light appears to be fairly uniform, with no obvious spiral arm structure or distinct features visible at this resolution. The galaxy shows minimal signs of disturbance and appears to be a relatively isolated system. The overall color suggests an older stellar population. The galaxy appears to be quite compact.
