The galaxy presents a primarily smooth morphology, appearing as an elliptical or lenticular structure. There is a notable central bulge exhibiting a concentrated region of higher luminosity. The galaxy displays an elongated, cigar-like shape, suggesting a deviation from a perfectly spherical form. The color gradient transitions from a bluer hue near the center to redder tones in the outer regions. There are no visible spiral arms or dust lanes; however, there appears to be a very slight disturbance indicating a potential minor merger in the galaxy's past. Overall, the galaxy does not appear to have a very high star formation rate.
