The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth light distribution. It is elongated, with a moderate degree of cigar-shapedness. There is a suggestion of a disturbed morphology, possibly indicating a past or ongoing interaction or merger event. The central region appears to be the brightest, with intensity gradually decreasing towards the outer edges. Colors range from a slightly bluish tint to a more central orange/red hue, perhaps indicating varying stellar populations and/or dust content within the galaxy. Although primarily smooth, there is some evidence of clumpy or irregular features especially surrounding the main body, which could be tidal debris or star-forming regions triggered by the interaction.
