The galaxy presents as an elongated, cigar-shaped structure. Its central region exhibits a diffuse, yellowish-white hue, possibly indicating a population of older stars. The galaxy's light profile appears relatively smooth across its major axis, suggesting a lack of prominent spiral arms. There is a notable redder component visible on the right side of the galaxy, possibly indicating a region of dust or older stellar populations. Overall, the galaxy appears to be relatively isolated and does not show obvious signs of major merger activity, though there may be minor tidal disturbances.
