The galaxy presents a smooth, elliptical morphology. Its overall shape appears to be somewhat elongated, leaning towards a cigar-like form, though a more intermediate elliptical shape is also plausible. A central bulge is clearly visible as a bright, concentrated region. The color profile suggests a relatively quiescent galaxy, dominated by older stellar populations, with the central bulge possibly displaying a bluer hue. No distinct spiral arms or active star-forming regions are discernible. There are no signs of major tidal disturbances or ongoing mergers with other galaxies, although minor disturbances cannot be entirely ruled out. The galaxy appears as an isolated system within its immediate vicinity.
