The object under examination appears to be a relatively distant galaxy, exhibiting a pronounced spindle or cigar-like morphology. Its overall color suggests a moderate population of older stars, with a smooth, featureless central bulge that is more luminous and yellowish in color. There is evidence of a faint, disklike structure extending outwards from the central bulge.

The disk itself is not well defined. There does not appear to be a prominent spiral arm structure, and the colors observed are consistent with low levels of ongoing star formation. Overall, the galaxy presents as an evolved system likely undergoing relatively slow stellar mass growth.
