The galaxy presents as a centrally concentrated object, likely an elliptical galaxy, viewed at a significant angle relative to its broadest axis. There is a clear bulge component with a yellow-orange color, suggesting an older stellar population and low levels of ongoing star formation. The galaxy appears relatively smooth, without prominent spiral arm structures or dust lanes visible in this image. Its overall shape is moderately elongated, tending toward cigar-shaped. There is no obvious evidence of major merging activity or significant tidal disturbances. The gradient of the bulge slowly dissipates into the surrounding space.