The galaxy appears to be a relatively smooth, elliptical type, exhibiting a concentrated central bulge. The light distribution suggests a spheroidal shape, more elongated than circular, but not extremely so. There is a distinct lack of defined spiral arm structures or prominent dust lanes. Coloration is mostly yellow, indicative of an older stellar population, but there may be the slight presence of blue around the edges, possibly suggesting some minimal recent star formation. Overall, the galaxy presents as a quiescent system with little evidence of ongoing major interactions.