The galaxy presents as a flattened spheroid, exhibiting a morphology consistent with an elliptical type. Its color gradient shows a central concentration of light, shifting towards redder hues in the core region, implying an older stellar population. The isophotes are relatively smooth, with no distinct spiral arm structure or dust lanes visible. The overall luminosity appears moderate, with no bright, actively star-forming regions detectable in this image. The galaxy's shape is elongated, closer to a cigar than a perfect circle. Possible minor disturbances in the galaxy's structure are present, however, no merging is present.
