The galaxy presents as an elliptical or lenticular type system, exhibiting a smooth, concentrated light distribution. The central region displays a significantly higher luminosity than the surrounding areas, suggesting a dense nucleus or bulge. The overall shape is elongated, with a cigar-like appearance. There is an absence of distinct spiral arms or significant dust lanes. Based on the color profile and the apparent lack of features indicative of active star formation, it is plausible that the galaxy is comprised primarily of an older stellar population, resulting in the slightly redder hue. There are hints of minor disturbances in the outer regions but nothing indicative of an ongoing major merger. The system appears relatively isolated.
