This galaxy appears to be an elliptical type, characterized by a smooth, relatively featureless light distribution. It exhibits a pronounced elongation, resembling a cigar shape. The central region is brighter and has a yellowish-white hue, suggesting an older stellar population. Moving outward, the color transitions to a more blueish-white, potentially indicative of some younger stars and/or a different mix of stellar metallicity. There's no strong evidence of spiral arms or significant dust lanes. There is a potential small disturbance or companion to the right of the galaxy, but it is difficult to say. Overall, the galaxy presents a quiescent appearance, consistent with a relatively low current star formation rate.
