This galaxy presents as a relatively smooth, elongated structure, likely a disk galaxy viewed at a high inclination. The central bulge appears prominent, exhibiting a concentrated brightness that decreases gradually towards the edges. The overall color appears to be dominated by older stellar populations, with a yellowish-red hue. There is little evidence of strong spiral arm structure or significant dust lanes, suggesting a morphology that is not dominated by active star formation. The shape is considerably elongated, resembling a cigar shape, indicating a high degree of ellipticity. The galaxy does not seem to be undergoing any major merging events or significant tidal disturbances; it displays a mostly undisturbed structure. It exhibits characteristics of a massive system with a moderate star formation rate.
