This galaxy presents a morphology characterized by a dominant smooth structure. The overall shape appears somewhat elliptical, exhibiting a moderate degree of roundness, tending toward an intermediate classification rather than a perfectly circular or elongated form. There is a faint disturbance noted in the galaxy, although no clear signs of ongoing major merging events are evident. The galaxy displays a distinct color gradient. A central bright region exhibits a yellowish-orange hue, suggestive of an older stellar population with relatively low rates of current star formation. The galaxy's substantial estimated mass suggests it is a relatively large and mature system. The red shift observed in the galaxy indicates that it is quite distant. The galaxy appears to be on the larger end of dwarf galaxies and/or on the smaller end of spirals.