The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its overall shape is elongated, appearing cigar-shaped rather than perfectly round. The color profile suggests a relatively old stellar population, with a dominant yellow hue and a lack of significant blue regions indicative of recent star formation. There is no strong evidence of spiral arm structure or a prominent disk. The galaxy appears isolated, without any indications of major mergers or strong tidal disturbances in its immediate vicinity, though there may be a faint hint of minor disturbances in its outer regions.
