The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elongated, appearing cigar-shaped. There may be evidence of a disk but it seems to be largely dominated by its bulge. The core region exhibits a brighter, slightly redder hue, which could indicate an older stellar population. The outer regions show hints of a bluer, albeit faint, distribution, suggesting the potential for some recent star formation, although this is not overtly pronounced. There are no strong indications of major merger events or tidal disturbances, though a minor interaction cannot be ruled out based on this imagery alone. The galaxy appears to be reasonably massive.
