This galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated light distribution. It possesses an elongated shape, with an apparent cigar-like morphology, but also has characteristics of being in between round and this elongated shape. There is a central bulge that seems to dominate the overall structure, contributing significantly to the galaxy's total luminosity. No prominent spiral arms or distinct dust lanes are visible within the observable bands. The color profile suggests a population of older stars and a general lack of active star formation, although a minor degree of ongoing activity cannot be entirely ruled out. Based on the apparent roundness and the even light distribution, the galaxy is most likely in a relatively isolated environment, showing little sign of recent or ongoing merger activity, beyond a negligible disturbance. The galaxy is observed at a redshift value that indicates it is a significant distance from us.
