The galaxy appears to be a relatively smooth, elongated structure. Its dominant color is reddish-orange, suggesting an older stellar population with a lower rate of ongoing star formation. The shape is not perfectly round, appearing more cigar-shaped. There is no clear evidence of spiral arms or a well-defined disk; the light is smoothly distributed across the galaxy’s body. There is no obvious sign of any major merger event or significant tidal disturbance affecting the overall morphology of the galaxy, though it is possible there is some minor asymmetry.
