The galaxy appears as an elongated, cigar-shaped structure, with its major axis oriented diagonally in the image. The light distribution is relatively smooth, with a concentrated central region transitioning into a fainter, extended halo or disk. The core exhibits a yellowish hue, potentially indicating an older stellar population. A faint bluish tinge is visible along the edges, possibly suggestive of more recent star formation or a population of hotter, younger stars. There is no obvious spiral arm structure, which makes it challenging to classify the morphological type beyond elliptical or lenticular. No signs of major disturbances such as tidal tails or irregular shapes are noted; the object appears to be in a relatively quiescent state, based on the light's current appearance.
