The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated distribution of light. The shape is elongated, displaying a cigar-like morphology, significantly deviating from a circular shape. It lacks a distinct spiral arm structure or prominent dust lanes, supporting its classification as an elliptical type. The color is primarily a yellow-red hue, suggesting an older stellar population with fewer young, massive stars. There is minimal evidence of ongoing major star formation or significant disturbances from mergers. The galaxy is generally isolated, showing no signs of recent or ongoing interaction with other galaxies.
