The galaxy appears as a moderately bright, elliptical-like object with a relatively smooth and concentrated central region. Its overall shape is elongated, exhibiting a cigar-like appearance, with a high degree of central concentration. The central region displays a yellowish hue, suggesting an older stellar population. The outer regions show a transition towards a more bluish tint, possibly indicating the presence of some younger stars. There is no distinct spiral arm structure or prominent dust lanes are visible. The galaxy does not seem to be undergoing any major merging events or exhibiting strong tidal disturbances, though some minor irregularities in the outer regions cannot be ruled out.
