The galaxy presents as a relatively smooth, elliptical-like structure. It appears elongated in shape, with a ratio of major to minor axis suggesting a cigar-like form. The central region exhibits a higher surface brightness, gradually decreasing towards the outer edges. The color profile displays a yellowish-red hue, indicative of an older stellar population with a lower proportion of young, blue stars and/or dust absorption. There is little indication of prominent spiral arms or significant active star formation regions within the visible spectrum. No obvious signs of tidal disruption or ongoing mergers are readily apparent from this image.
